Low Temperature Opacities

Abstract

Previous computations of low temperature Rosseland and Planck mean opacities from Alexander & Ferguson (1994) are updated and expanded. The new computations include a more complete equation of state with more grain species and updated optical constants. Grains are now explicitly included in thermal equilibrium in the equation of state calculation, which allows for a much wider range of grain compositions to be accurately included than was previously the case. The inclusion of high temperature condensates such as Al${}_2$O${}_3$ and CaTiO${}_3$ significantly affects the total opacity over a narrow range of temperatures before the appearance of the first silicate grains. The new opacity tables are tabulated for temperatures ranging from 30000 K to 500 K with gas densities from 10${}^{-4}$ g cm${}^{-3}$ to 10${}^{-19}$ g cm${}^{-3}$. Comparisons with previous Rosseland mean opacity calculations are discussed. At high temperatures, the agreement with OPAL and Opacity Project is quite good. Comparisons at lower temperatures are more divergent as a result of differences in molecular and grain physics included in different calculations. The computation of Planck mean opacities performed with the opacity sampling method are shown to require a very large number of opacity sampling wavelength points; previously published results obtained with fewer wavelength points are shown to be significantly in error. Methods for requesting or obtaining the new tables are provided.

39 pages with 12 figures. To be published in ApJ, April 2005

References in corpus (8)

• The Limiting Effects of Dust in Brown Dwarf Model Atmospheres
• Rosseland and Planck Mean Opacities for Protoplanetary Discs
• Model Atmospheres for M (Sub)Dwarfs: I. The base model grid
• TiO and H${}_2$O absorption lines in cool stellar atmospheres
• Dust Grain-Size Distributions From MRN to MEM
• A comparison of Rosseland-mean opacities from OP and OPAL
• The Molecular Line Opacity of MgH in Cool Stellar Atmospheres
• Analysis of Keck High Resolution Spectra of VB10

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• Pre-main-sequence isochrones -- III. The Cluster Collaboration isochrone server
• Effect of coronal temperature on the scale of solar chromospheric jets
• Fundamental properties of five Kepler stars using global asteroseismic quantities and ground-based observations
• Stellar convective penetration: parameterized theory and dynamical simulations
• Solar Models with Revised Abundances and Opacities
• Effective temperatures of red giants in the APOKASC catalogue and the mixing length calibration in stellar models
• Signatures of Circumstellar Interaction in the Type IIL Supernova ASASSN-15oz
• Lithium depletion is a strong test of core-envelope recoupling
• Asteroseismology of 36 Kepler subgiants -- II: Determining ages from detailed modelling
• Stellar models with the ML2 theory of convection
• The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
• Multidimensional realistic modelling of Cepheid-like variables. I: Extensions of the ANTARES code
• Outbursts in Global Protoplanetary Disk Simulations
• On rapid binary mass transfer -- I. Physical model
• Obtaining Precision Constraints on Modified Gravity with Helioseismology
• Survey of non-linear hydrodynamic models of type-II Cepheids
• CoRoT 102918586: a Gamma Dor pulsator in a short period eccentric eclipsing binary
• Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: I. Adiabatic properties
• The Absolute Age of M92
• Nucleosynthesis of binary-stripped stars
• Asteroseismology of 3,642 Kepler Red Giants: Correcting the Scaling Relations based on Detailed Modeling
• Disc formation and fragmentation using radiative non-ideal magnetohydrodynamics
• Coupled Thermal and Compositional Evolution of Photo Evaporating Planet Envelopes
• A grid of 1D low-mass star formation collapse models
• Evolutionary models for R Coronae Borealis stars
• SpaceInn hare-and-hounds exercise: Estimation of stellar properties using space-based asteroseismic data
• Kepler Observations of the Asteroseismic Binary HD 176465
• Confronting uncertainties in stellar physics II. exploring differences in main-sequence stellar evolution tracks
• HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2
• Globular Cluster Abundances from High-Resolution, Integrated-Light Spectroscopy. III. The Large Magellanic Cloud: Fe and Ages
• Accretion disks around massive stars: Hydrodynamic structure, stability and dust sublimation
• Mean density inversions for red giants and red clump stars
• The coupling between internal waves and shear-induced turbulence in stellar radiation zones: the critical layer
• Does misalignment between magnetic field and angular momentum enhance or suppress circumstellar disk formation?
• Models of solar surface dynamics: impact on eigenfrequencies and radius
• Limits on the 2.2 microns contrast ratio of the close orbiting planet HD 189733b
• Evolution models of helium white dwarf--main sequence star merger remnants
• Evolutionary modelling of subdwarf B stars using MESA with the predictive mixing and convective premixing schemes
• Combining radiative transfer and diffuse interstellar medium physics to model star formation
• Carbon-Oxygen Phase Separation in MESA White Dwarf Models
• Constraints on the distance moduli, helium and metal abundances, and ages of globular clusters from their RR Lyrae and non-variable horizontal-branch stars. II. Multiple stellar populations in 47Tuc, M3, and M13
• Progenitor Model of SN 1987A Based on the Slow Merger Scenario
• Formation, orbital and thermal evolution, and survival of planetary-mass clumps in the early phase of circumstellar disk evolution
• A Progenitor for the Extremely Luminous Type Ic Supernova 2007bi
• On the Spectral Evolution of Hot White Dwarf Stars. II. Time-dependent Simulations of Element Transport in Evolving White Dwarfs with STELUM
• Combining multiple structural inversions to constrain the Solar modelling problem
• A prescription for the asteroseismic surface correction
• On the asymptotic acoustic-mode phase in red-giant stars and its dependence on evolutionary state
• Differential rotation in main-sequence solar-like stars: Qualitative inference from asteroseismic data
• Constraining massive star activities in the final years through properties of supernovae and their progenitors
• 3D simulations of M star atmosphere velocities and their influence on molecular FeH lines
• Numerical experiments to help understand cause and effect in massive star evolution
• Multigroup radiation hydrodynamics with flux-limited diffusion and adaptive mesh refinement
• Impact of helium diffusion and helium-flash-induced carbon production on gravity-mode pulsations in subdwarf B stars
• Towards a unified model of stellar rotation
• Fundamental properties of Kepler and CoRoT targets: III. Tuning scaling relations using the first adiabatic exponent
• The masses of retired A stars with asteroseismology: Kepler and K2 observations of exoplanet hosts
• Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly II: Stellar Evolution and Asteroseismic Applications
• A high resolution spectral atlas of brown dwarfs
• The Preservation of Super Earths and the Emergence of Gas Giants after Their Progenitor Cores have Entered the Pebble Isolation Phase
• A New, Efficient Stellar Evolution Code for Calculating Complete Evolutionary Tracks
• Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly I: A New Standard Solar Model
• Surface effects on the red giant branch
• An Extended Grid of Nova Models. III. Very Luminous, Red Novae
• Variation of Stellar Envelope Convection and Overshoot with Metallicity
• Morphological effects on IR band profiles: Experimental spectroscopic analysis with application to observed spectra of oxygen-rich AGB stars
• Infrared High-Resolution Integrated Light Spectral Analyses of M31 Globular Clusters from APOGEE
• Pulsation properties of ultra-massive DA white dwarf stars with ONe cores
• A Near-infrared RR Lyrae census along the southern Galactic plane: the Milky Way's stellar fossil brought to light
• Hydrogen in hot subdwarfs formed by double helium white dwarf mergers
• Generalised form factor dark matter in the Sun
• Habitable Zones and UV Habitable Zones around Host Stars
• A detailed study of the main sequence of the Globular Cluster NGC 6397: can we derive constraints on the existence of multiple population?
• Optically Thin Core Accretion: How Planets Get Their Gas in Nearly Gas-Free Disks
• The cosmic carbon footprint of massive stars stripped in binary systems
• Helium settling in F stars: constraining turbulent mixing using observed helium glitch signature
• The Evolution of Rotation and Magnetic Activity in 94 Aqr Aa from Asteroseismology with TESS
• In-depth study of 16CygB using inversion techniques
• Evolutionary models for ultracool dwarfs
• Surface convection and red giants radii measurements
• The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
• Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
• Stellar Nucleosynthesis in the Hyades Open Cluster
• Enhancement of Lithium in Red Clump Stars by the Additional Energy Loss Induced by New Physics
• Filling the Black Hole Mass Gap: Avoiding Pair Instability in Massive Stars through Addition of Non-Nuclear Energy
• Investigating surface correction relations for RGB stars
• Cumulative theoretical uncertainties in lithium depletion boundary age
• Testing stellar evolution models with the retired A star HD 185351
• Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution
• S stars and s-process in the Gaia era I. Stellar parameters and chemical abundances in a sub-sample of S stars with new MARCS model atmospheres
• Evolutionary and pulsation properties of Type II Cepheids
• Constraints on the structure of 16 Cyg A and 16 Cyg B using inversion techniques
• Lithium in LP 944-20
• Benchmarking the Multi-dimensional Stellar Implicit Code MUSIC
• Tess asteroseismology of the known planet host star ${\lambda }^2$ Fornacis
• An Atlas of Convection in Main-Sequence Stars
• LAMOST Time-Domain Survey: First Results of four $K$2 plates
• Constraining a Model of Turbulent Coronal Heating for AU Microscopii with X-Ray, Radio, and Millimeter Observations
• Tests of the asymptotic large frequency separation of acoustic oscillations in solar-type and red giant stars
• A Theoretical Study of Acoustic Glitches in Low-Mass Main-Sequence Stars
• Constraining transport of angular momentum in stars: Combining asteroseismic observations of core helium burning stars and white dwarfs
• Impact of convection and resistivity on angular momentum transport in dwarf novae
• Low-Temperature Gas Opacities with AESOPUS 2.0
• Higher metal abundances do not solve the solar problem
• An Explosive End to Intermediate-Mass Zero-Metallicity Stars and Early Universe Nucleosynthesis
• Binary evolution along the Red Giant Branch with BINSTAR: The barium star perspective
• Latitudinal differential rotation in the solar analogues 16 Cyg A and B
• Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771
• Surface-effect corrections for the solar model
• Characterizing two solar-type Kepler subgiants with asteroseismology: KIC10920273 and KIC11395018
• Recycling of the first atmospheres of embedded planets: Dependence on core mass and optical depth
• Global 3D Radiation Hydrodynamic Simulations of Proto-Jupiter's Convective Envelope
• Evolutionary implications of the new triple-alpha nuclear reaction rate for low mass stars
• Stellar Photospheric Abundances as a Probe of Disks and Planets
• First solar models with OPAS opacity tables
• The p-process in exploding rotating massive stars
• Modeling the Asteroseismic Surface Term across the HR Diagram
• Gravitational settling in pulsating subdwarf B stars and their progenitors
• The very low mass multiple system LHS\,1070 -- a testbed for model atmospheres for the lower end of the main sequence
• Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
• On the necessity of composition-dependent low-temperature opacity in metal-poor AGB stars
• Terzan 5: an alternative interpretation for the split horizontal branch
• Multiple populations in massive star clusters under the magnifying glass of photometry: Theory and tools
• Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
• The evolution of white dwarfs resulting from helium-enhanced, low-metallicity progenitor stars
• Pulsational instabilities driven by the $\epsilon$ mechanism in hot pre-horizontal branch stars I. The Hot-Flasher Scenario
• On the structure and evolution of planets and their host stars $-$ effects of various heating mechanisms on the size of giant gas planets
• Asteroseismic determination of fundamental parameters of sun-like stars using multi-layered neural networks
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• Mass Transfer and Stellar Evolution of the White Dwarfs in AM CVn Binaries
• Reversing the verdict: Cataclysmic variables could be the dominant progenitors of AM CVn binaries after all
• Modeling Kepler Observations of Solar-like Oscillations in the Red-giant Star HD 186355
• Mitigating the mass dependence in the $\Delta \nu$ scaling relation of red-giant stars
• An explanation for the gap in the Gaia HRD for M dwarfs
• The puzzle of metallicity and multiple stellar populations in the Globular Clusters in Fornax
• Theoretical uncertainties on the radius of low- and very-low mass stars
• From the CMD of Omega Centauri and (super-)AGB stellar models to a Galactic plane passage gas purging chemical evolution scenario
• Helium White Dwarfs in Cataclysmic Variables
• S-process in low-mass extremely metal-poor stars
• The evolution of ultra-massive carbon oxygen white dwarfs
• Detailed AGB evolutionary models and near infrared colours of intermediate-age stellar populations: Tests on star clusters
• Towards a new era in giant exoplanet characterisation
• Spherical-shell boundaries for two-dimensional compressible convection in a star
• Nonlinear outcome of gravitational instability in an irradiated protoplanetary disc
• Solar Models with Revised Abundance
• Pulsating low-mass white dwarfs in the frame of new evolutionary sequences: II. Nonadiabatic analysis
• SNAPSHOT: Connections between Internal and Surface Properties of Massive Stars
• In-situ star formation in accretion disk and explanation for correlation between black hole mass and metallicity in AGNs
• Magnetic and Rotational Evolution of $\rho$ CrB from Asteroseismology with TESS
• Absolute parameters for AI Phoenicis using WASP photometry
• Convective-core overshoot and suppression of oscillations: Constraints from red giants in NGC6811
• Asteroseismic modelling of solar-type stars: A deeper look at the treatment of initial helium abundance
• Determining the metallicity of the solar envelope using seismic inversion techniques
• Core-Envelope Coupling in Intermediate-Mass Core-Helium Burning Stars
• Observational Constraints Upon Cool Disk Material in Quiescent Black Hole Binaries
• Turbulent and wind-driven accretion in dwarf novae threaded by a large scale magnetic field
• Average opacity calculation for core-collapse supernovae
• Sound-speed inversion of the Sun using a nonlocal statistical convection theory
• Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer
• Imprint of planet formation in the deep interior of the Sun
• Asteroseismology of hybrid $\delta$ Scuti--$\gamma$ Doradus pulsating stars
• Magnetic geometry and surface differential rotation of the bright Am star Alhena A
• Thorough characterisation of the 16 Cygni system Part I: Forward seismic modelling with WhoSGlAd
• Hydrodynamical modeling of the light curves of core collapse supernovae with HYPERION. I. The mass range 13-25 Msun, the metallicities -3<=[Fe/H]<=0 and the case of SN1999em
• The Nature of Millisecond Pulsars with Helium White Dwarf Companions
• Seismic modeling of a very young SPB star -- KIC8264293
• The subgiant HR 7322 as an asteroseismic benchmark star
• The $\beta$ Cep/SPB star 12 Lacertae: extended mode identification and complex seismic modelling
• Chemically-dissected rotation curves of the Galactic Bulge from Main Sequence proper motions
• Testing Angular Momentum Transport and Wind Loss in Intermediate Mass Core Helium Burning Stars
• Theoretical oscillation frequencies for solar-type dwarfs from stellar models with $⟨3\mathrm{D}⟩$-atmospheres
• Linear Solar Models
• Testing Metal Poor Stellar Models and Isochrones with HST Parallaxes of Metal Poor Stars
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• Hierarchically modelling Kepler dwarfs and subgiants to improve inference of stellar properties with asteroseismology
• Asteroseismic modelling of the metal-poor star Tau Ceti
• Searching for dark energy with the Sun
• WIYN Open Cluster Study LXII: Comparison of Isochrone Systems using Deep Multi-Band Photometry of M35
• KIC 10736223: An Algol-type eclipsing binary just undergone the rapid mass-transfer stage
• Fundamental properties of nearby stars and the consequences on DeltaY/DeltaZ
• Realistic Simulations of Stellar Surface Convection with ANTARES: I. Boundary Conditions and Model Relaxation
• The birth and early evolution of a low mass protostar
• Optical TiO and VO band emission in two embedded protostars: IRAS 04369+2539 and IRAS 05451+0037
• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• Modeling overcontact binaries, I. The effect of tidal deformation
• A synthetic sample of short-cadence solar-like oscillators for TESS
• A differential chemical abundance scale for the globular cluster M5
• The HST large programme on $\omega$ Centauri -- V. Exploring the Ultracool Dwarf Population with Stellar Atmosphere and Evolutionary Modelling
• Calibrating the updated overshoot mixing model on eclipsing binary stars: HY Vir, YZ Cas, X2 Hya & VV Crv
• Applications of the $k$-$\omega$ model in stellar evolutionary models
• The Radius and Entropy of a Magnetized, Rotating Fully-convective Star: Analysis With Depth-dependent Mixing Length Theories
• Examining the Relationship Between Convective Core Overshoot and Stellar Properties Using Asteroseismology
• On the existence of brown dwarfs more massive than the hydrogen burning limit
• Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters
• The Asteroseismic Imprints of Mass Transfer: A Case Study of a Binary Mass Gainer in the SPB Instability Strip
• A differential chemical element analysis of the metal poor Globular Cluster NGC 6397
• Asteroseismology and interferometry of the red giant star epsilon Oph
• Modeling contact binaries, II. The effect of energy transfer
• Quiescent nuclear burning in low-metallicity white dwarfs
• The chemical composition of TS 01, the most oxygen-deficient planetary nebula. AGB nucleosynthesis in a metal-poor binary star
• Comparison of two- and three-dimensional compressible convection in a pre-main sequence star
• Giant planet formation: episodic impacts vs. gradual core growth
• The evolutionary status of the blue hook stars in Omega Centauri
• Convection Enhances Magnetic Turbulence in AM CVn Accretion Disks
• A theoretical framework of BL Her stars. I. Effect of metallicity and convection parameters on period-luminosity and period-radius relations
• Apsidal motion in the massive binary HD 152248 -- Constraining the internal structure of the stars
• The robustness of asteroseismic estimates of global stellar parameters to surface term corrections
• Polarization in microlensing towards the Galactic bulge
• Evidence for Cluster to Cluster Variations in Low-Mass Stellar Rotational Evolution
• Chemical Abundance Evidence of Enduring High Star Formation Rates in an Early Type Galaxy: High [Ca/Fe] in NGC 5128 Globular Clusters
• Isochrone fitting to the open cluster M67 in the era of Gaia and improved model physics
• Formation of redbacks via accretion induced collapse
• Is Thermohaline Mixing the Full Story? Evidence for Separate Mixing Events near the Red Giant Branch Bump
• Evolutionary status of Polaris
• Pre-supernova mixing in CEMP-no source stars
• Core radii and common-envelope evolution
• Carbon Rich Extremely Metal Poor Stars: Signatures of Population-III AGB stars in Binary Systems
• Comprehensive stellar seismic analysis : New method exploiting the glitches information in solar-like pulsators
• Evidence of structural discontinuities in the inner core of red-giant stars
• Radiative Acceleration of Dense Circumstellar Material in Interacting Supernovae
• Overcoming the structural surface effect with a realistic treatment of turbulent convection in 1D stellar models
• Aldebaran b's temperate past uncovered in planet search data
• A Bayesian estimation of the helioseismic solar age
• The eclipsing binary systems with $\delta$ Scuti component. I. KIC 10661783
• Dark matter capture and annihilation in stars: Impact on the red giant branch tip
• Protostellar Disk Evolution Over Million-Year Timescales with a Prescription for Magnetized Turbulence
• AE Ursae Majoris -- a $\delta$ Scuti Star in the Hertzsprung Gap
• The Pulsation Properties of $\lambda$ Bootis Stars I. The Southern TESS Sample
• Heavy Elements Nucleosynthesis On Accreting White Dwarfs: building seeds for the p-process
• Impact of Convective Boundary Mixing on the TP-AGB
• Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances
• Detection of Solar-Like Oscillations, Observational Constraints, and Stellar Models for $\theta$ Cyg, the Brightest Star Observed by the {\it Kepler} Mission
• The Effect of Metallicity-Dependent T-tau Relations on Calibrated Stellar Models
• Surface layer independent model fitting by phase matching: theory and application to HD49933 an HD177153 (aka Perky)
• Optimal Integrated Abundances for Chemical Tagging of Extragalactic Globular Clusters
• Photophoretic Structuring of Circumstellar Dust Disks
• Asteroseismology and Spectropolarimetry of the Exoplanet Host Star $\lambda$ Serpentis
• Observational predictions for Thorne-Żytkow objects
• On the Color-Metallicity Relation of the Red Clump and the Reddening Toward the Magellanic Clouds
• The effects of a revised ${}^7$Be e${}^{-}$-capture rate on solar neutrino fluxes
• Convection and rotation boosted prescription of magnetic braking: application to the formation of extremely low-mass white dwarfs
• Theoretical seismic properties of pre-main sequence gamma Doradus pulsators
• Effects of continuum fudging on non-LTE synthesis of stellar spectra. I. Effects on estimates of UV continua and Solar Spectral Irradiance variability
• Electric heating and angular momentum transport in laminar models of protoplanetary disks
• The implications of large binding energies of massive stripped core collapse supernova progenitors on the explosion mechanism
• Asteroseismology of the Double-Mode High-Amplitude $\delta$ Scuti Star VX Hydrae
• Hydrodynamics and survivability during post-main-sequence planetary engulfment
• Comparing the Effect of Radiative Transfer Schemes on Convection Simulations
• On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres
• Common Envelope Evolution of Massive Stars
• Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors
• Effects of Alpha-Element Enhancement and the Thermally Pulsing-Asymptotic Giant Branch on Surface Brightness Fluctuation Magnitudes and Broadband Colors
• Asteroseismic constraints on Asymmetric Dark Matter: Light particles with an effective spin-dependent coupling
• Testing abundance-age relations beyond solar analogues with Kepler LEGACY stars
• Kepler-93: a testbed for detailed seismic modelling and orbital evolution of super-earths around solar-like stars
• Automated determination of g-mode period spacing of red-giant stars
• Mending the structural surface effect of 1D stellar structure models with non-solar metallicities based on interpolated 3D envelopes
• 3D Stagger model atmospheres with FreeEOS I. Exploring the impact of microphysics on the Sun
• Probability Distribution of Terrestrial Planets in Habitable Zones around Host Stars
• Robust asteroseismic properties of the bright planet host HD 38529
• HD 179949b: A Close Orbiting Extrasolar Giant Planet with a stratosphere?
• Testing Asteroseismic Radii of Dwarfs and Subgiants with Kepler and Gaia
• On a new parameter to estimate the helium content in old stellar systems
• Close stellar encounters at the Galactic Centre I: The effect on the observed stellar populations
• Regular frequency patterns in the classical delta Scuti star HD 144277 observed by the MOST satellite
• The Role of Dust in Models of Population Synthesis
• Solar models with new low-metal abundances
• Dissecting the microphysics behind the metallicity-dependence of massive stars radii
• Time-dependent, long-term hydrodynamic simulations of the inner protoplanetary disk I: The importance of stellar magnetic torques
• Bridging the Gap between Intermediate and Massive Stars I: Validation of MESA against the State-of-the-Art Monash Stellar Evolution Program for a 2$M_{\odot }$ AGB Star
• Rotation at the Fully Convective Boundary: Insights from Wide WD + MS Binary Systems
• Stellar Evolution and Tidal Dissipation in REBOUNDx
• Stellar evolution models with overshooting based on 3-equation non-local theories, II. Main-sequence models of A- and B-type stars
• Chemical mixing in low mass stars: I. Rotation against atomic diffusion including radiative accelerations
• Characterizing Observed Extra Mixing Trends in Red Giants using the Reduced Density Ratio from Thermohaline Models
• Addressing the acoustic tachocline anomaly and the lithium depletion problem at the same time
• The Linkage between the Core Mass and the Magnetic Field of an Extrasolar Giant Planet from Future Radio Observations
• Asteroseismology of KIC 7107778: a binary comprising almost identical subgiants
• Pulsational instability of pre-main-sequence models from accreting protostars II. Modelling echelle diagrams of $\delta$ Scuti stars without rotational splitting
• Modelling fully convective stars in eclipsing binaries: KOI-126 and CM Draconis
• Asteroseismic analysis of the CoRoT target HD49933
• Asteroseismic analysis of solar-mass subgiants KIC 6442183 and KIC 11137075 observed by Kepler
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• BESTP -- An Automated Bayesian Modeling Tool for Asteroseismology
• $\alpha$ Centauri A as a potential stellar model calibrator: establishing the nature of its core
• Fundamental properties of a selected sample of Ap stars: Inferences from interferometric and asteroseismic constraints
• Improved calibration of the radii of cool stars based on 3D simulations of convection: implications for the solar model
• Analysis of the linear approximation of seismic inversions for various structural pairs
• Gravito-turbulence in irradiated protoplanetary discs
• Grid-based seismic modelling at high and low signal-to-noise ratios HD 181420 and HD 175272
• Asteroseismic analysis of two alpha-enhanced stars KIC 7976303 and KIC 8694723
• Seismic analysis of the double-mode radial pulsator SX Phoenicis
• The IACOB project: IV. New predictions for high-degree non-radial mode instability domains in massive stars and connection with macroturbulent broadening
• Asteroseismic inversions for radial differential rotation of Sun-like stars: ensemble fits
• Impact of magnetic activity on inferred stellar properties of main sequence Sun-like stars
• An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models
• The evolution of low mass, close binary systems with a neutron star component: a detailed grid
• Sink particle radiative feedback in smoothed particle hydrodynamics models of star formation
• The dynamical mass and evolutionary status of the type-II Cepheid in the eclipsing binary system OGLE-LMC-T2CEP-211 with a double-ring disk
• In Situ and Ex Situ Formation Models of Kepler 11 Planets
• The impact of composition choices on solar evolution: age, helio- and asteroseismology, and neutrinos
• A hadronic emission model for black hole-disc impacts in the blazar OJ 287
• Structural and Evolutionary Diagnostics from Asteroseismic Phase Functions
• The impact of the uncertainties in the 12C(α,γ)16O reaction rate on the evolution of low- to intermediate-mass stars
• A Transparent Window into Early-Type Stellar Variability
• Pulsations powered by hydrogen shell burning in white dwarfs
• Exploring the convective core of the hybrid $\delta$ Scuti-$\gamma$ Doradus star CoRoT 100866999 with asteroseismology
• Asteroseismology of the $\delta$ Scuti star HD 50844
• Stellar evolution models with entropy-calibrated mixing-length parameter: application to red giants
• Modeling of multimode radially pulsating High-Amplitude Delta Scuti stars from the OGLE Galactic bulge sample
• Further evidence of saturated, boosted, and disrupted magnetic braking from evolutionary tracks of cataclysmic variables
• Helium-Abundance and Other Composition Effects on the Properties of Stellar Surface Convection in Solar-like Main-sequence Stars
• Helioseismic and Neutrino Data Driven Reconstruction of Solar Properties
• The statistical properties of protostellar discs and their dependence on metallicity
• Seismic analysis of HD43587Aa, a solar-like oscillator in a multiple system
• New light on the driving mechanism in roAp stars. Part I. Effects of metallicity
• Measuring Polarization in microlensing events
• Ages of 70 dwarfs of three populations in the solar neighborhood: considering O and C abundances in stellar models
• Seismic Solar Models from Ledoux discriminant inversions
• Fundamental properties of solar-like oscillating stars from frequencies of minimum $\Delta \nu$: I. Model computations for solar composition
• The effect of the adiabatic assumption on asteroseismic scaling relations for luminous red giants
• Titanium and Iron in the Cassiopeia A Supernova Remnant
• Platform for Probing Radiation Transport Properties of Hydrogen at Conditions Found in the Deep Interiors of Red Dwarfs
• The solar abundance problem: the effect of the turbulent kinetic flux on the solar envelope model
• Constraints on the properties of macroscopic transport in the Sun from combined lithium and beryllium depletion
• Models of Metal-Poor Stars with Different Initial Abundances of C, N, O, Mg, and Si. I. Bolometric Corrections Derived from New MARCS Synthetic Spectra and Their Implications for Observed Colour-Magnitude Diagrams
• Polarization in binary microlensing events
• An upper limit on the spins of merging binary black holes formed through binary evolution
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Low-mass pre--main-sequence stars in the Magellanic Clouds
• Galactic vs. Extragalactic Origin of the Peculiar Transient SCP 06F6
• Formation of low mass protostars and their circumstellar disks
• Tracing the evolution of short-period binaries with super-synchronous fast rotators
• Updated Pre-Main Sequence tracks at low metallicities for 0.1< M/Mo<1.5
• Li-rich and super Li-rich giants produced by element diffusion
• A need to revise stellar opacities from asteroseismology of $\delta$ Scuti stars
• The effect of including molecular opacities of variable composition on the evolution of intermediate-mass AGB stars
• A discontinuity in the luminosity-mass relation and fluctuations in the evolutionary tracks of low-mass and low-metallicity stars at the Gaia M-dwarf gap
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• On the inference of stellar ages and convective-core properties in main-sequence solar-like pulsators
• Standard solar models: a perspective from updated solar neutrino fluxes and the gravity-mode period spacing
• The extremely low metallicity star SDSS J102915+172927: a subgiant scenario
• The YNEV stellar evolution and oscillation code
• The influence of metallicity on a combined stellar and disk evolution
• Gray Radiation Hydrodynamics with the FLASH Code for Astrophysical Applications
• AME - Asteroseismology Made Easy. Estimating stellar properties by use of scaled models
• Asteroseismic modelling strategies in the PLATO era I. Mean density inversions and direct treatment of the seismic information
• From Theory to Observations and viceversa: theoretical uncertainties and observational constraints
• Impact of the new solar abundances on the calibration of the PMS binary system RS Cha
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• The Massive M31 Cluster G1: Detailed Chemical Abundances from Integrated Light Spectroscopy
• Characterising abundance-age relations of GALAH stars using oxygen-enhanced stellar models
• Revisiting the Red-giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters
• The 2003-4 multisite photometric campaign for the Beta Cephei and eclipsing star 16 (EN) Lacertae with an Appendix on 2 Andromedae, the variable comparison star
• Frequency identification and asteroseismic analysis of the red giant KIC 9145955: fundamental parameters and helium core size
• A simple scheme to implement a nonlocal turbulent convection model for the convective overshoot mixing
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Expanding the Catalog: Considering the Importance of Carbon, Magnesium, and Neon in the Evolution of Stars and Habitable Zones
• Optab: Public code for generating gas opacity tables for radiation hydrodynamics simulations
• Elimination of the Blue Loops in the Evolution of Intermediate-mass Stars by the Neutrino Magnetic Moment and Large Extra Dimensions
• Bayesian inference of stellar parameters based on 1D stellar models coupled with 3D envelopes
• Stellar Parameters of Main Sequence Turn-off Star Candidates Observed with the LAMOST and Kepler
• Impact of the physical processes in the modeling of HD49933
• The Influence of Disk Composition on the Evolution of Stars in the Disks of Active Galactic Nuclei
• Simulating a stellar contact binary merger -- I. Stellar models
• Radiation Magnetohydrodynamic Simulations of Protostellar Collapse: Low-Metallicity Environments
• A binary with a $\delta$~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821
• Nucleosynthetic yields of intermediate-mass primordial to extremely metal-poor stars
• Solar Models with dynamic screening and early mass loss tested by helioseismic, astrophysical, and planetary constraints
• The mass and age of the first SONG target: the red giant 46 LMi
• Seismic characterization of red giants going through the Helium-core flash
• MONTAGE: AGB nucleosynthesis with full s-process calculations
• Assessing the processes behind planet engulfment and its imprints
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• Grids of stellar models including second harmonic and colours: Solar composition
• Uncovering the chemical structure of the pulsating low-mass white dwarf SDSS J115219.99+024814.4
• A well-balanced scheme for the simulation tool-kit A-MaZe: implementation, tests, and first applications to stellar structure
• Magnetic Archaeology of Early-Type Stellar Dynamos
• Period Change Rates of Large Magellanic Cloud Cepheids using MESA
• Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries
• Can very massive stars avoid Pair-Instability Supernovae?
• Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri
• Mode identification and seismic study of $\delta$ Scuti, the prototype of a class of pulsating stars
• Birth of magnetized low-mass protostars and circumstellar disks
• Impact of asteroseismology on improving stellar ages determination
• Uncertainties and systematics in stellar evolution models of Red Giant Stars
• The effective temperature -- radius relationship of M-dwarfs
• Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge
• Radiative transfer in circumstellar disks - I. 1D models for GQ Lupi
• Grain Physics and Rosseland Mean Opacities
• Asteroseismic analysis of 15 solar-like oscillating evolved stars
• Modelling stars with Gaussian Process Regression: Augmenting Stellar Model Grid
• Matching the frequency spectrum of PMS stars by means of standard and rotating models
• Vertical Convection in Turbulent Accretion Disks and Light Curves of the A0620-00 1975 Outburst
• Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
• On the Anti-Correlation between Duration and Redshift in Gamma-ray Bursts
• Evolution models of helium white dwarf--main-sequence star merger remnants: the mass distribution of single low-mass white dwarfs
• Rotating Solar Models in Agreement with Helioseismic Results and Updated Neutrino Fluxes
• Core overshoot constrained by the absence of a solar convective core and some solar-like stars
• What governs the spin distribution of very young < 1 Myr low mass stars
• On the relevance of bubbles and potential flows for stellar convection
• Updated High-Temperature Opacities for the Dartmouth Stellar Evolution Program and their Effect on the Jao Gap Location
• A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
• Yunnan-III models for Evolutionary population synthesis
• Asteroseismic Inversions for Internal Sound Speed Profiles of Main-sequence Stars with Radiative Cores
• The Secular Periodic Evolution of X-ray Quasi-periodic Eruptions Driven by Star-disc Collisions
• The Evolution of Binaries Embedded Within Common Envelopes
• The age of the Methuselah star in light of stellar evolution models with tailored abundances
• On the importance of wave planet interactions for the migration of two super-Earths embedded in a protoplanetary disk
• Implications of a turbulent convection model for classical Cepheids
• The fate of rotating massive stars across cosmic times
• The Interior Structure Constants as an Age Diagnostic for Low-Mass, Pre-Main Sequence Detached Eclipsing Binary Stars
• Evolutionary history of four binary blue stragglers from the globular clusters ωCen, M55, 47 Tuc and NGC 6752
• Astrophysics in 2005
• Isochrones of M67 with an Expanded Set of Parameters
• Asteroseismic investigation on KIC 10526294 to probe convective core overshoot mixing
• Frequency dependence of the large frequency separation of solar-like oscillators: Influence of the Helium second-ionization zone
• The initial mass-remnant mass relation for core collapse supernovae
• Differential Rotation in Convective Envelopes: Constraints from Eclipsing Binaries
• The effects of individual metal contents on isochrones for C, N, O, Na, Mg, Al, Si, and Fe
• Determining the evolutionary stage of the delta Scuti star HIP 80088 with asteroseismology
• Comparing the asteroseismic properties of pulsating pre-extremely low mass white dwarf and delta Scuti stars
• Seismic diagnostics of solar-like oscillating stars
• WASP 0639-32: a new F-type subgiant/K-type main-sequence detached eclipsing binary from the WASP project
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests
• Two-Dimensional Radiation-Hydrodynamic Simulations of Luminous Red Novae
• Modeling of two CoRoT solar analogues constrained by seismic and spectroscopic analysis
• Radiation Hydrodynamics Simulations of Spherical Protostellar Collapse for Very Low Mass Objects
• TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet
• HIP 15429: A newborn Be star on an eccentric binary orbit
• Testing a non-local 1-equation turbulent convection model: A solar model
• The core degenerate scenario for the type Ia supernova SN 2020eyj
• On the nature of the core of $\alpha$ Centauri A: the impact of the metallicity mixture
• Overview and Validation of the Asteroseismic Modeling Portal v2.0
• Structure of the solar photosphere studied from the radiation hydrodynamics code ANTARES
• The preliminary statistical analysis of LAMOST DR8 low resolution AFGK stars
• Recent Advances in Modeling Stellar Interiors
• Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
• Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?
• Terminating a common envelope jets supernova impostor event with a super-Eddington blue supergiant
• Suggested magnetic braking prescription derived from field complexity fails to reproduce the cataclysmic variable orbital period gap
• Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
• Pushing the boundaries of asteroseismic individual frequency modelling: unveiling two evolved very-low metallicity red giants
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• Asteroseismology of the pre-main-sequence $\delta$ Scuti pulsator IP Persei
• Numerical integral of resistance coefficients in diffusion
• The implications of a companion enhanced wind on millisecond pulsar production
• A revisit to the enigmatic variable star 21 Comae
• A Possible Mechanism for Driving Oscillations in Hot Giant Planets
• High contrast imaging with Fizeau interferometry: The case of Altair
• Performance of the Stellar Abundances and atmospheric Parameters Pipeline adapted for M dwarfs I. Atmospheric parameters from the spectroscopic module
• An evolutionary model for V404 Cyg system
• Asteroseismic analysis of eight solar-like oscillating evolved stars in the open cluster NGC 6811
• Asteroseismology of double-mode radial $\delta$ Scuti stars: AE Ursae Majoris and RV Arietis
• Constraints on stellar parameters of the SPB star HD182255 from complex asteroseismology
• The efficiency of mixed modes for angular momentum transport
• The Initial Magnetic Field Distribution in AB Stars
• Solar Models and Astrophysical S-factors Constrained by Helioseismic Results and Updated Neutrino Fluxes
• Stellar evolution and modelling stars
• The double helium-white dwarf channel for the formation of AM CVn binaries
• The convective kissing instability in low-mass M-dwarf models: convective overshooting, semi-convection, luminosity functions, surface abundances and star cluster age dating
• Revisiting Kepler-444 Part I. Seismic modelling and inversions of stellar structure
• Photospheric Opacity and Over-Expanded Envelopes of Asymptotic Giant Branch Stars
• Asteroseismic Investigations of the Binary System HD176465
• Protoplanetary disks around magnetized young stars with large-scale magnetic fields I: Steady-state solutions
• The role of detailed gas and dust opacities in shaping the evolution of the inner disc edge subject to episodic accretion
• Revisiting the extremely long-period cataclysmic variables V479 Andromedae and V1082 Sagitarii
• The structure and evolution of a high-mass stellar merger in the Hertzsprung gap
• The evolutionary and asteroseismic imprints of mass accretion. The 10 M${}_{\odot }$ $\beta$ Cep case study
• Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215.82+111745.0: a model with $p$-mode pulsations consistent with the observations
• Semiconvective Mixing in Low-Mass Stars
• Asteroseismic Structure Inversions of Main-Sequence Solar-like Oscillators with Convective Cores
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• On the use of the average large separation in surface layer independent model fitting
• MAISTEP -- a new grid-based machine learning tool for inferring stellar parameters I. Ages of giant-planet host stars
• Precise determination of fundamental parameters of six exoplanet host stars and their planets
• Discovery of new magnetic δ Scuti stars and impact of magnetism on pulsation excitation
• Evolutionary models for the Very Massive Stars in the R136 cluster of 30 Doradus in the Large Magellanic Cloud
• Seismic detection of core magnetic fields in red giants using the gravity offset
• Off-centre convective zones in mass accreting stellar models
• Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
• Properties of observable mixed inertial and gravito-inertial modes in γ Doradus stars
• Neutrinos and Asteroseismology of Stars over the Helium Flash
• On the effect of pulsar evaporation on the cooling of white dwarfs
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• Turbulent viscosity by convection in accretion discs - a self-consistent approach
• Solar models with protosolar accretion and turbulent mixing
• Asteroseismic modelling of the Binary HD 176465
• Toward a Comprehensive Grid of Cepheid Models with MESA II. Impact of Physical and Numerical Assumptions on Elemental Abundances
• Asteroseismic stellar modelling: systematics from the treatment of the initial helium abundance
• Numerical simulations of line-profile variation beyond a single-surface approximation for oscillations in roAp stars
• Chameleon fields and solar physics
• Using Lithium and Beryllium to Study Structure and Evolution of Rotating Stars
• Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
• The depletion of the red supergiant envelope radiative zone during common envelope evolution
• Metallicity Ceiling in Quasars from Recycled Stellar Winds
• Habitable Zones of Host Stars During the Post-MS Phase
• Analysis of accretion disc structure and stability using open code for vertical structure
• Seismic study of solar convection and overshooting: results of nonlocal convection
• Realising efficient computation of individual frequencies for red-giant models
• Core-Collapse Supernovae: From Neutrino-Driven 1D Explosions to Light Curves and Spectra
• Asteroseismology of low-mass stars: the balance between partial ionisation and Coulomb interactions
• Coronal heating problem solution by means of axion origin photons
• The impact of the transport of chemicals and electronic screening on helioseismic and neutrino observations in solar models
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• Solar radius and luminosity variations induced by the internal dynamo magnetic fields
• Theoretical study of $\gamma$ Doradus pulsations in pre-main sequence stars
• A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
• Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Exploring the Small-scale Magnetic Fields in the Atmosphere of HD 49385 by Asteroseismic Analysis
• Challenges in Solar and Stellar Model Physics
• Horizontal branch structure, age, and chemical composition for very metal-poor extragalactic globular clusters
• Continuous Habitable Zones: Using Bayesian Methods to Prioritize Characterization of Potentially Habitable Worlds
• Glitch analysis and asteroseismic modelling of subgiant $\mu$ Herculis: confirming and interpreting the ${\Gamma }_1$ peak as the helium glitch
• Influence of the Outer Boundary Condition on models of AGB stars
• Frequency dependence of Delta_nu of solar-like oscillators investigated: Influence of HeII ionization zone
• Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
• New theoretical predictions on Type II Cepheids: towards a self consistent Pop. II distance scale
• The Age of the KIC 7177553 System
• Exploring the physical properties of the $\gamma$ Dor binary star RX Dra with photometry and asteroseismology
• Comparative study of low-temperature opacities with GARSTEC models
• New insight on Young Stellar Objects accretion shocks -- a claim for NLTE opacities
• He-enriched STAREVOL models for globular cluster multiple populations. Self-consistent isochrones from ZAMS to the TP-AGB phase
• Revisiting the exoplanet radius valley with host stars from SWEET-Cat
• Instability of Population III Black Hole Accretion Disks
• Variations of helioseismic parameters due to magnetic field generated by a flux transport model
• The effect of late giant collisions on the atmospheres of protoplanets and the formation of cold sub-Saturns
• Discs and outflows in the early phases of massive star formation: influence of magnetic fields and ambipolar diffusion
• PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators
• OO Dra: an Algol-type binary formed through an extremely helium-poor mass accretion revealed by asteroseismology
• The final fates of close hot subdwarf - white dwarf binaries: mergers involving He/C/O white dwarfs and the formation of unusual giant stars with C/O-dominated envelopes
• Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
• Can small-scale magnetic fields be the major cause for the near-surface effect of the solar p-mode frequencies?
• Magnetic dynamos in white dwarfs -III: explaining the occurrence of strong magnetic fields in close double white dwarfs
• Convective Penetration in Early-Type Stars
• Ages of Main-Sequence Turn-Off Stars from the GALAH Survey
• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
• Thermomagnetic Ettingshausen-Nernst effect in tachocline, magnetic reconnection phenomenon in lower layers, axion mechanism of solar luminosity variations, coronal heating problem solution and mechanism of ADM variations around BH
• Advanced asteroseismic modelling: breaking the degeneracy between stellar mass and initial helium abundance
• Towards solar measurements of nuclear reaction rates
• What Determines the Brightness of the Magnetically Open Solar Corona?: Insights from Three-dimensional Radiative Magnetohydrodynamic Simulations and Observations
• Constraints on the Axion-Photon Coupling Using Stellar Modelling
• Discerning internal conditions of pulsating hot subdwarf B stars. Modelling multiple trapped modes in KIC 10001893
• Probing stellar cores from inversions of frequency separation ratios
• Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection
• Anti-Solar Differential Rotation May Have Revived Magnetic Braking in the Subgiant 31 Aquilae
• Asteroseismic Analysis of a Red Giant KIC 9145955 by Including the Small-scale Magnetic Fields in the Atmosphere
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Testing the 3-equation Kuhfuss Convection Model using the Sun
• Evolution of the ZTF SLRN-2020 star-planet merger
• The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars
• Radial differential rotation leading to dipole collapse in pre-main-sequence stars
• Resonance locking and tidal evolution in rotating γ-Doradus binaries