Scaled solar tracks and isochrones in a large region of the Z-Y plane. II. From 2.5 to 20 solar masses

Abstract

We extend our theoretical computations for low-mass stars to intermediate-mass and massive stars, for which few databases exist in the literature. Evolutionary tracks and isochrones are computed from 2.50 to 20 solar masses for agrid of 37 chemical compositions with metal content Z between 0.0001 and 0.070 and helium content Y between 0.23 and 0.40. Synthetic TP-AGB models allow stellar tracks and isochrones to be extended until the end of the thermal pulses along the AGB. We provide software tools for the bidimensional interpolation (in Y and Z) of the isochrones. We present tracks for scaled-solar abundances and the corresponding isochrones from very old ages down to about 10 million years. The extension of the blue loops and the instability strip of Cepheid stars are compared and the Cepheid mass-discrepancy is discussed. The location of red supergiants in the H-R diagram is in good agreement with the evolutionary tracks for masses from 10 to 20 solar masses. Tracks and isochrones are available in tabular form for the adopted grid of chemical compositions in the extended plane Z-Y in three photometric systems. An interactive web interface allows users to obtain isochrones of any chemical composition inside the provided Z-Y range and also to simulate stellar populations with different Y(Z) helium-to-metal enrichment laws.

17 pages, 18 figures, accepted for publication in A&A

References in corpus (15)

• Star Formation Histories, Abundances and Kinematics of Dwarf Galaxies in the Local Group
• Helioseismology and Solar Abundances
• Scaled solar tracks and isochrones in a large region of the Z-Y plane I. From the ZAMS to the TP-AGB end for 0.15 - 2.5 Mo stars
• Evolution of asymptotic giant branch stars I. Updated synthetic TP-AGB models and their basic calibration
• The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars
• Rotational mixing in massive binaries: detached short-period systems
• The influence of chemical composition on the properties of Cepheid stars. II-The iron content
• The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity
• On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation
• A critical test of empirical mass loss formulae applied to individual giants and supergiants
• Cepheid Mass-loss and the Pulsation -- Evolutionary Mass Discrepancy
• New period-luminosity and period-color relations of classical Cepheids: III. Cepheids in SMC
• On the solar nickel and oxygen abundances
• On the effect of helium enhancement on bolometric corrections and Teff-colour relations
• The Physical Properties of Red Supergiants: Comparing Theory and Observations

Cited by in corpus (175)

• PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
• Mind your Ps and Qs: the Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars
• A new generation of PARSEC-COLIBRI stellar isochrones including the TP-AGB phase
• New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey
• PARSEC evolutionary tracks of massive stars up to $350M_{\odot }$ at metallicities 0.0001$\le Z\le$0.04
• BANYAN. XI. The BANYAN $\Sigma$ multivariate Bayesian algorithm to identify members of young associations within 150 pc
• Determining stellar atmospheric parameters and chemical abundances of FGK stars with iSpec
• New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star forming dwarf galaxies
• Galacticus: A Semi-Analytic Model of Galaxy Formation
• Gaia FGK Benchmark Stars: Effective temperatures and surface gravities
• A catalogue of young runaway Hipparcos stars within 3kpc from the Sun
• Interrelated Main-Sequence Mass-Luminosity, Mass-Radius and Mass-Effective Temperature Relations
• On the Age and Binarity of Fomalhaut
• A luminous, blue progenitor system for a type-Iax supernova
• Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code. II. The Southern Clusters and Overview
• Main-Sequence Effective Temperatures from a Revised Mass-Luminosity Relation Based on Accurate Properties
• Core crystallization and pile-up in the cooling sequence of evolving white dwarfs
• The Besancon Galaxy model renewed I. Constraints on the local star formation history from Tycho data
• Insights into the content and spatial distribution of dust from the integrated spectral properties of galaxies
• Insights into the Cepheid distance scale
• Exploring Anticorrelations and Light Element Variations in Northern Globular Clusters Observed by the APOGEE Survey
• Calibrations of Atmospheric Parameters Obtained from the First Year of SDSS-III APOGEE Observations
• Chemical Abundances in Field Red Giants from High-Resolution H-Band Spectra using the APOGEE Spectral Linelist
• Planetary Construction Zones in Occultation: Discovery of an Extrasolar Ring System Transiting a Young Sun-like Star and Future Prospects for Detecting Eclipses by Circumsecondary and Circumplanetary Disks
• A comparison of evolutionary tracks for single Galactic massive stars
• Relative merits of different types of rest-frame optical observations to constrain galaxy physical parameters
• Atmospheric Characterization of the Hot Jupiter Kepler-13Ab
• Chemical element ratios of SDSS early-type galaxies
• The Pisa Stellar Evolution Data Base for low-mass stars
• Optically visible post-AGB/RGB stars and young stellar objects in the Small Magellanic Cloud: candidate selection, spectral energy distributions and spectroscopic examination
• Magnetic field topology of the unique chemically peculiar star CU Virginis
• The masses, and the mass discrepancy of O-type stars
• Optically Visible Post-AGB Stars, Post-RGB Stars and Young Stellar Objects in the Large Magellanic Cloud
• Spitzer Evidence for a Late Heavy Bombardment and the Formation of Urelites in η Corvi at ~1 Gyr
• A Kine-Chemical Investigation of the AB Dor Moving Group "Stream"
• Age Determination for 346 Nearby Stars in the Herschel DEBRIS Survey
• On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
• A WISE Survey of Circumstellar Disks in Taurus
• A newly discovered stellar type: dusty post-red giant branch stars in the Magellanic Clouds
• Effects of Helium Enrichment in Globular Clusters I.Theoretical Plane with PGPUC stellar evolution code
• Possible Detection of the Stellar Donor or Remnant for the Type Iax Supernova 2008ha
• Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3
• Physics of Eclipsing Binaries. IV. The impact of interstellar extinction on the light curves of eclipsing binaries
• Mean age gradient and asymmetry in the star formation history of the Small Magellanic Cloud
• HR 5907: Discovery of the most rapidly rotating magnetic B-type star by the MiMeS Collaboration
• Massive star evolution : rotation, winds, and overshooting vectors in the Mass-Luminosity plane I. A calibrated grid of rotating single star models
• Lithium-rich giants in the Galactic thick disk
• The Kappa Andromedae System: New Constraints on the Companion Mass, System Age & Further Multiplicity
• Cumulative physical uncertainty in modern stellar models I. The case of low-mass stars
• On the evolutionary and pulsation mass of Classical Cepheids: III. the case of the eclipsing binary Cepheid CEP0227 in the Large Magellanic Cloud
• The Star Formation History of the Solar Neighbourhood from the White Dwarf Luminosity Function
• Resolved photometry of extragalactic young massive star clusters
• Does the Debris Disk around HD 32297 Contain Cometary Grains?
• Establishing binarity amongst Galactic RV Tauri stars with a disc
• The Close Binary Properties of Massive Stars in the Milky Way and Low-Metallicity Magellanic Clouds
• The Birth of an Ultra-Luminous X-ray Source in M83
• Gaia FGK Benchmark Stars: New Candidates At Low-Metallicities
• The Effect of Tides on the Population of PN from Interacting Binaries
• Uncertainties in grid-based estimates of stellar mass and radius. SCEPtER: Stellar CharactEristics Pisa Estimation gRid
• Constraints on the origin of the massive, hot, and rapidly rotating magnetic white dwarf RE J 0317-853 from an HST parallax measurement
• A nearby recent supernova that ejected the runaway star zeta Oph, the pulsar PSRB1706-16, and 60-Fe found on Earth
• Habitable Zones of Post-Main Sequence Stars
• Comparative Modelling of the Spectra of Cool Giants
• The Water Abundance of the Directly Imaged Substellar Companion κ And b Retrieved from a Near Infrared Spectrum
• Thick disk kinematics from RAVE and the solar motion
• On the Blue Loops of Intermediate-Mass Stars
• Large-scale environments of binary AGB stars probed by Herschel - I. Morphology statistics and case studies of R Aquarii and W Aquilae
• The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B
• 3D hydrodynamical CO5BOLD model atmospheres of red giant stars: I. Atmospheric structure of a giant located near the RGB tip
• On the Progenitor System of the Type Iax Supernova 2014dt in M61
• Star Formation History in two fields of the Small Magellanic Cloud Bar
• A method to estimate stellar ages from kinematical data
• The $\mu$ Tau Association: A 60 Myr-Old Coeval Group at 150 pc from the Sun
• Evidence for Temperature Change and Oblique Pulsation from Light Curve Fits of the Pulsating White Dwarf GD 358
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• The connection between missing AGB stars and extended horizontal branches
• Uniform Forward-Modeling Analysis of Ultracool Dwarfs. I. Methodology and Benchmarking
• Extrasolar Refractory-Dominated Planetesimals: an Assessment
• Recovery of the Historical SN1957D in X-rays with Chandra
• Fundamental parameters of 16 late-type stars derived from their angular diameter measured with VLTI/AMBER
• HD 183648: a Kepler eclipsing binary with anomalous ellipsoidal variations and a pulsating component
• A New Class of Nascent Eclipsing Binaries with Extreme Mass Ratios
• Further investigation of white dwarfs in the open clusters NGC2287 and NGC3532
• Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C
• CRIRES-POP: A library of high resolution spectra in the near-infrared
• The Progenitors and Lifetimes of Planetary Nebula
• The sdA problem - III. New extremely low-mass white dwarfs and their precursors from Gaia astrometry
• Early-type Eclipsing Binaries with Intermediate Orbital Periods
• The sdA problem I: Physical Properties
• The Puzzling Li-rich Red Giant Associated with NGC 6819
• Not-So-Simple Stellar Populations in the Intermediate-age Large Magellanic Cloud Star Clusters NGC 1831 and NGC 1868
• The Penn State - Toruń Centre for Astronomy Planet Search stars IV. Dwarfs and the complete sample
• MASCARA-4 b/bRing-1b - A retrograde hot Jupiter around the bright A3V star HD 85628
• Searching for Planets in Holey Debris Disks with the Apodizing Phase Plate
• Dwarf spheroidal satellites of M31: I. Variable stars and stellar populations in Andromeda XIX
• Calibrating convective-core overshooting with eclipsing binary systems. The case of low-mass main-sequence stars
• Eccentric Ellipsoidal Red Giant Binaries in the LMC: Complete Orbital Solutions and Comments on Interaction at Periastron
• Magnetic field topology and chemical spot distributions in the extreme Ap star HD 75049
• Ultra Long Period Cepheids: a primary standard candle out to the Hubble flow
• Theory of stellar convection: Removing the Mixing-Length Parameter
• Exploring an Alternative Channel of Evolution Towards SNa Ia Explosion
• The evolutionary nature of RV Tauri stars in the SMC and LMC
• Chemical abundances of two extragalactic young massive clusters
• Atmospheric composition of weak G band stars: CNO and Li abundances
• A search for pulsations in the HgMn star HD 45975 with CoRoT photometry and ground-based spectroscopy
• New infrared spectral indices of luminous cold stars: from early K to M-types
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• Imaging an 80 AU Radius Dust Ring Around the F5V Star HD 157587
• On the post-common-envelope central star of the planetary nebula NGC 2346
• Spiral arm kinematics for Milky Way stellar populations
• Type II Cepheids Pulsating in the First Overtone from the OGLE Survey
• The Role of Dust in Models of Population Synthesis
• Cosmic Star Formation: a simple model of the SFRD(z)
• GalMod: a Galactic synthesis population model
• Constraining the Thin Disc Initial Mass Function using Galactic Classical Cepheids
• Carbon and Oxygen abundances across the Hertzsprung gap
• Galactic structure in the outer disk: the field in the line of sight to the intermediate-age open cluster Tombaugh 1
• Chlorine Abundances in Cool Stars
• Theory of Stellar Population Synthesis with an application to N-Body simulations
• Chlorine Isotope Ratios in M Giants
• What planetary nebulae tell us about helium and the CNO elements in Galactic bulge stars
• Turbulent convection and pulsation stability of stars - III. Non-adiabatic oscillations of red giants
• Composite Stellar Populations and Element by Element Abundances in the Milky Way Bulge and Elliptical Galaxies
• Constraining the subgrid physics in simulations of isolated dwarf galaxies
• Star formation in the S233 region
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• Modeling and Analysis of a Spectrum of the Globular Cluster NGC 2419
• BRITE-Constellation photometry of $\bpi^5$ Orionis, an ellipsoidal SPB variable
• Atmospheres and UV Environments of Earth-like Planets Throughout Post-Main Sequence Evolution
• Study of extremely reddened AGB stars in the Galactic bulge
• Component masses of young, wide, non-magnetic white dwarf binaries in the SDSS DR7
• Chemical Abundances in the Globular Clusters NGC 6229 and NGC 6779
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• Impact of distance determinations on Galactic structure. II. Old tracers
• A Closer Look at the Alpha Persei Coronal Conundrum
• On the delay times of merging double neutron stars
• Theory of stellar convection II: first stellar models
• GK Car and GZ Nor: Two low-luminous, depleted RV Tauri stars
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Colour-magnitude diagram in simulations of galaxy formation
• The progenitors of magnetic white dwarfs in open clusters
• On Disentangling IMF Degeneracies in Integrated Light
• UBVI CCD Photometry of the Open Cluster NGC 4609 and Hogg 15
• The Galactic Chemical Evolution of Chlorine
• The Fate of Oceans on First-Generation Planets Orbiting White Dwarfs
• Stellar physical parameters from Str ömgren photometry. Application to the young stars in the Galactic anticenter survey
• VI-Band Follow-Up Observations of Ultra-Long-Period Cepheid Candidates in M31
• Stellar population astrophysics (SPA) with the TNG -- The chemical content of the red supergiant population in the Perseus complex
• On the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth
• Study of Eclipsing Binary and Multiple Systems in OB Associations II. The Cygnus OB Region: V443 Cyg, V456 Cyg and V2107 Cyg
• Dissipative phenomena in extended-bodies interactions I: Methods Dwarf galaxies of the Local Group and their synthetic CMDs
• Systematic trend of water vapour absorption in red giant atmospheres revealed by high resolution TEXES 12 micron spectra
• Thermally Pulsing Asymptotic Giant Branch Star Models and Globular Cluster Planetary Nebulae I: The Model
• A Bound on the Light Emitted During the TP-AGB Phase
• The Angular Diameter and Effective Temperature of the Lithium-Rich K Giant HD 148293 from the CHARA Array
• Individual element sensitivity for stellar evolutionary isochrones
• MagAO Imaging of Long-period Objects (MILO). II. A Puzzling White Dwarf around the Sun-like Star HD 11112
• Magellanic Cloud stars with TiO bands in emission: binary post-RGB/AGB stars or young stellar objects?
• New Radial Velocities for 30 Candidate Runaway Stars and a Possible Binary Supernova Origin for HIP 9470 and PSR J0152-1637
• The multiplicity of ϕ Phe revisited
• Three nearby K-giants with planets: Accurate determination of basic parameters, including an analysis of metallicity based on Fe I lines
• Environmental effects on star formation in dwarf galaxies and star clusters
• Is the young star cluster NGC 376 dissolving in the field of the SMC?
• A new framework for understanding the evolution of early-type galaxies
• On distinguishing age from metallicity with photometric data
• On the impact of Helium abundance on the Cepheid Period-Luminosity and Wesenheit relations and the Distance Ladder
• Discovery of pulsating components in eclipsing binary systems through the TESS light curves: The cases of CPD-30 740, HD 97329, V1637 Ori and TYC 683-640-1
• The orbital elements and physical properties of the eclipsing binary BD+36 3317, a probable member of $\delta$ Lyr cluster
• Evolutionary and hydrodynamic models of short--period Cepheids
• The Predicted Properties of Helium-Enriched Globular Cluster Progenitors at High Redshift
• No Open Cluster in the Ruprecht 93 Region
• Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
• High resolution observations of Cen A: Yellow and red supergiants in a region of jet-induced star formation?
• Four New Eclipsing Binary Systems in the TESS field: CD-34 13220, HD 295082, TYC 6484-426-1 and TYC 6527-2310-1
• Six Newly Discovered Eclipsing Binary Systems in the TESS field