OP data on CD for mean opacities and radiative accelerations

Abstract

All monochromatic opacity data from the Opacity Project (OP), together with all codes required for the calculation of mean opacities and radiative accelerations for any required chemical mixture, temperature and mass-density, are being put on a 700 Mb CD which will be made generally available. The present paper gives a concise summary of the contents of the CD. More complete documentation will be provided on the CD itself.

4 pages, 2 figures, submitted to MNRAS

References in corpus (2)

• A comparison of Rosseland-mean opacities from OP and OPAL
• On the importance of inner-shell transitions for opacity calculations

Cited by in corpus (52)

• Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
• Internal mixing of rotating stars inferred from dipole gravity modes
• Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry
• Asteroseismology and Interferometry
• An asteroseismic study of the beta Cephei star theta Ophiuchi: constraints on global stellar parameters and core overshooting
• Solar structure and evolution
• Instability strips of SPB and beta Cephei stars: the effect of the updated OP opacities and of the metal mixture
• The two hybrid B-type pulsators: Nu Eridani and 12 Lacertae
• Shock breakout theory
• Convection Causes Enhanced Magnetic Turbulence in Accretion Disks in Outburst
• Gravity-mode pulsations in subdwarf B stars: a critical test of stellar opacity
• Helium abundance in a sample of cool stars: measurements from asteroseismology
• Evolution of Thermally Pulsing Asymptotic Giant Branch Stars IV. Constraining Mass-Loss & Lifetimes of Low Mass, Low Metallicity AGB Stars
• Asteroseismic estimate of helium abundance of a solar analog binary system
• Modelling Long-Period Variables - I. A new grid of O-rich and C-rich pulsation models
• Domains of pulsational instability of low-frequency modes in rotating upper main-sequence stars
• Atlas of solar hidden photon emission
• Quantifying uncertainties in the solar axion flux and their impact on determining axion model parameters
• Amplitude variability or close frequencies in pulsating stars? The Delta Scuti star FG Vir
• Radiative Cooling in MHD Models of the Quiet Sun Convection Zone and Corona
• Helium settling in F stars: constraining turbulent mixing using observed helium glitch signature
• Solar and Stellar Photospheric Abundances
• Equation of state for partially ionized carbon and oxygen mixtures at high temperatures
• Asteroseismic determination of fundamental parameters of sun-like stars using multi-layered neural networks
• Asteroseismic modelling of solar-type stars: A deeper look at the treatment of initial helium abundance
• Seismic modelling of early B-type pulsators observed by BRITE: I. $\theta$ Ophiuchi
• Seismic modeling of a very young SPB star -- KIC8264293
• Helium line emissivities in the solar corona
• Axions as a probe of solar metals
• On The Impact Of 22Ne On The Pulsation Periods Of Carbon-Oxygen White Dwarfs With Helium Dominated Atmospheres
• Physics of Thermonuclear Explosions: Magnetic Field Effects on Deflagration Fronts and Observable Consequences
• Asteroseismology of the double-radial mode $\delta$ Scuti star BP Pegasi
• Searching for a solar relaxion/scalar with XENON1T and LUX
• Seismic analysis of the double-mode radial pulsator SX Phoenicis
• An improved parametric method for evaluating radiative accelerations in stellar interiors
• Plasma opacity calculations using the Starrett and Saumon average-atom model with ion correlations
• An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models
• A need to revise stellar opacities from asteroseismology of $\delta$ Scuti stars
• BRITE observations of $\nu$ Centauri and $\gamma$ Lupi, the first non-eclipsing members of the new class of nascent binaries
• Mode identification and seismic study of $\delta$ Scuti, the prototype of a class of pulsating stars
• Core overshoot constrained by the absence of a solar convective core and some solar-like stars
• Self-Excited Pulsations and the Instability Strip of Long-Period Variables: the Transition from Small-Amplitude Red Giants to Semi-Regular Variables
• Asteroseismology of double-mode radial $\delta$ Scuti stars: AE Ursae Majoris and RV Arietis
• Recent Advances in Modeling Stellar Interiors
• Complex asteroseismology of the hybrid B-type pulsator $\gamma$ Pegasi: a test of stellar opacities
• K2 Observations of 95 Vir: delta Scuti Pulsations in a Chromospherically Active Star
• The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations
• Asteroseismology of sz lyn using multi-band high time resolution photometry from ground and space
• On the Observability of Optically Thin Coronal Hyperfine Structure Lines
• Chemical element transport in stellar evolution models
• Atomic data activities by the OP and IP consortia: past, present and new perspectives within the VAMDC
• PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators