Red Giant Branch Stars: The Theoretical Framework
暂无分享,去创建一个
S. Cassisi | M. Salaris | A. Weiss | S. Cassisi | A. Weiss | A. Weiss | M. Salaris
[1] D. Hayes,et al. Calibration of Fundamental Stellar Quantities , 1985 .
[2] C. Claver,et al. DDO Photometry of M71: Carbon and Nitrogen Patterns among Evolving Giants , 2001, astro-ph/0108121.
[3] C. Sneden,et al. 12C/13C in metal-poor field halo giants , 2001 .
[4] T. Bedding. Fundamental stellar properties: the interaction between observation and theory. Poster proceedings. , 1997 .
[5] M. Shetrone,et al. New Analyses of Star-to-Star Abundance Variations among Bright Giants in the Mildly Metal-poor Globular Cluster M5 , 2001, astro-ph/0106249.
[6] L. Girardi,et al. Evolutionary sequences of stellar models with new radiative opacities. VI. $Z=0.0001$ , 1996 .
[7] K. Swamy. Profiles of strong lines in K- dwarfs , 1966 .
[8] Taft E. Armandroff,et al. Standard Globular Cluster Giant Branches in the (M(I), (V - I)o) Plane , 1990 .
[9] D. G. Hummer,et al. The equation of state for stellar envelopes. III - Thermodynamic quantities , 1988 .
[10] C. Claver,et al. Carbon Abundances of M92 Red Giant Branch Stars , 2001 .
[11] R. Gilliland,et al. K Giants in 47 Tucanae: Detection of a New Class of Variable Stars , 1996 .
[12] R. Zinn,et al. The horizontal-branch stars in globular clusters. I - The period-shift effect, the luminosity of the horizontal branch, and the age-metallicity relation , 1990 .
[13] A. Weiss,et al. Standard and Nonstandard Plasma Neutrino Emission Revisited , 1994 .
[14] M. Catelán. Horizontal-Branch Models and the Second-Parameter Effect. III. The Impact of Mass Loss on the Red Giant Branch and the Case of M5 and Palomar 4/Eridanus , 1999, astro-ph/9910334.
[15] R. G. Gratton,et al. The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters , 2001 .
[16] E. Friel,et al. ON THE CARBON ABUNDANCE OF SUBGIANT STARS IN THE GLOBULAR CLUSTER M 92. , 1985 .
[17] Y.-W. Lee,et al. Toward Better Age Estimates for Stellar Populations: The Y2 Isochrones for Solar Mixture , 2001 .
[18] European Southern Observatory,et al. A Step toward the Calibration of the Red Giant Branch Tip as a Standard Candle , 2001, astro-ph/0104114.
[19] P. Demarque,et al. The luminosity function on the subgiant branch of 47 Tucanae A comparison of observation and theory , 1984 .
[20] L. Girardi,et al. Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 , and from to 0.03 , 1999, astro-ph/9910164.
[21] H. Iyetomi,et al. Electrical and thermal conductivities of dense matter in the liquid metal phase. I - High-temperature results , 1983 .
[22] Forrest J. Rogers,et al. Opal equation-of-state tables for astrophysical applications , 1996 .
[23] A. Sweigart,et al. Meridional circulation and CNO anomalies in red giant stars , 1979 .
[24] M. Catelán,et al. A superwind from early post-red giant stars? , 2001, astro-ph/0111295.
[25] D. VandenBerg,et al. The Luminosity Function of M30: Evidence for Rapidly Rotating Cores in the Cluster Giants? , 1998 .
[26] G. Worthey. Comprehensive stellar population models and the disentanglement of age and metallicity effects , 1994 .
[27] F. Kupka,et al. Convection in the atmospheres and envelopes of turnoff and giant branch stars of globular clusters , 2001 .
[28] J. Fernie,et al. RELATIONSHIPS BETWEEN THE JOHNSON AND KRON-COUSINS VRI PHOTOMETRIC SYSTEMS. , 1983 .
[29] Santiago Arribas,et al. The effective temperature scale of giant stars (F0–K5) - II. Empirical calibration of versus colours and [Fe/H] , 1999 .
[30] H. E. DeWitt,et al. Screening Factors for Nuclear Reactions. 11. Intermediate Screen-Ing and Astrophysical Applications , 1973 .
[31] A. Gußmann. B. BASCHEK, W. H. KEGEL, G. TRAVING (eds.) : Problems in Stellar Atmospheres and Envelopes. Springer‐Verlag, Berlin‐Heidelberg‐New‐York, 1975. XIX + 375 Seiten. Preis DM 48.‐ , 1976 .
[32] Judith G. Cohen,et al. Calibration of the CH and CN Variations Among Main-Sequence Stars in M71 and in M13 , 2001, astro-ph/0104099.
[33] D. Hatzidimitriou,et al. Advances in Stellar Evolution , 1997 .
[34] G. González,et al. Elemental Abundances in Giants in NGC 3201, a Globular Cluster with a Retrograde Orbit , 1998 .
[35] I. M. Schwarzschild,et al. RED GIANTS OF POPULATION II. IV , 1962 .
[36] D. Sugimoto,et al. Why Stars Become Red Giants , 2000 .
[37] A. Sweigart,et al. Evolutionary sequences for red giant stars , 1978 .
[38] Wendy L. Freedman,et al. The Tip of the Red Giant Branch as a Distance Indicator for Resolved Galaxies , 1993 .
[39] Jeff Secker,et al. Constraints on the Hubble constant from observations of the brightest red-giant stars in a Virgo-cluster galaxy , 1998, Nature.
[40] N. Suntzeff,et al. Carbon and nitrogen abundances in giant stars of the metal-poor globular cluster M15. , 1983 .
[41] G. Worthey,et al. Color‐Color Relations for Red Giants in Star Clusters , 1998, astro-ph/9804001.
[42] Towards the absolute planes: a new calibration of the bolometric corrections and temperature scales for Population II giants , 1998, astro-ph/9804297.
[43] Robert M. Cavallo,et al. Proton-Capture Nucleosynthesis in Globular Cluster Red Giant Stars , 1997, astro-ph/9708099.
[44] A catalogue of helium abundance indicators from globular cluster photometry , 1999, astro-ph/9911237.
[45] B. Paczynski,et al. Cluster AgeS Experiment: The Age and Distance of the Globular Cluster ω Centauri Determined from Observations of the Eclipsing Binary OGLEGC 17 , 2000, astro-ph/0012493.
[46] G. Costa. Abundance Anomalies in Globular Clusters , 1997 .
[47] M. Shetrone. Magnesium and carbon isotopes in globular cluster giants. Tests of deep mixing. II , 1996 .
[48] A. Sweigart. Effects of Helium Mixing on the Evolution of Globular Cluster Stars , 1997 .
[49] N. Grevesse,et al. In: Origin and Evolution of the elements , 1993 .
[50] Judith G. Cohen,et al. Infrared photometry, bolometric luminosities and effective temperatures for giant stars in 26 globular clusters. , 1983 .
[51] S. Djorgovski,et al. On the Helium Content of Galactic Globular Clusters via the R-Parameter , 2000, astro-ph/0003004.
[52] Helioseismology and standard solar models , 1996, astro-ph/9612053.
[53] M. S. Cooper,et al. Screening factors for nuclear reactions. I. General theory , 1973 .
[54] Russell D. Cannon,et al. Carbon and nitrogen abundance variations on the main sequence of 47 Tucanae , 1998 .
[55] THE GIANT, HORIZONTAL, AND ASYMPTOTIC BRANCHES OF GALACTIC GLOBULAR CLUSTERS. I. THE CATALOG, PHOTOMETRIC OBSERVABLES, AND FEATURES , 1999, astro-ph/9906248.
[56] R. J. Dickens,et al. Carbon abundances in red giant stars in the globular clusters M92 and NGC 6397 , 1979 .
[57] N. Itoh,et al. Neutrino Energy Loss in Stellar Interiors , 1985 .
[58] M. Schwarzschild,et al. Hydrogen Mixing by Helium-Shell Flashes , 1967 .
[59] J. Mengel,et al. Possible effects of internal rotation in low-mass stars , 1976 .
[60] G. Piotto,et al. Comparison between Predicted and Empirical [FORMULA][F]ΔV[SUP][RM]bump[/RM][/SUP][INF][RM]HB[/RM][/INF][/F][/FORMULA] in Galactic Globular Clusters , 1999 .
[61] D. Reimers. Circumstellar Envelopes and Mass Loss of Red Giant Stars , 1975 .
[62] G. Bono,et al. The Shape of the Red Giant Branch Bump as a Diagnostic of Partial Mixing Processes in Low-Mass Stars , 2001, astro-ph/0110247.
[63] I. Iben,et al. Hydrogen Burning and Dredge-up during the Major Core Helium Flash in a Z = 0 Model Star , 1990 .
[64] F. Silvestri,et al. Luminosity Functions for Globular Clusters , 1998 .
[65] Kiyoshi Katō,et al. Flash-assisted Deep Mixing in Globular Cluster Red Giants , 2001 .
[66] E. Guinan,et al. Theory and Tests of Convection In Stellar Structure , 1999 .
[67] I. Iben. On Why Intermediate-Mass Stars Become Giants after the Exhaustion of Hydrogen in Their Cores , 1993 .
[68] I. Goldman,et al. Stellar Turbulent Convection: A Self-consistent Model , 1996 .
[69] T. Lejeune,et al. A standard stellar library for evolutionary synthesis , 1998 .
[70] G. Raffelt. Core mass at the helium flash from observations and a new bound on neutrino electromagnetic properties , 1990 .
[71] C. Tout,et al. On a physical mechanism for extra mixing in globular cluster red giants , 2000 .
[72] I. Iben. Age and Initial Helium Abundance of Stars in the Globular Cluster M15 , 1968, Nature.
[73] G. A. Rutledge,et al. GALACTIC GLOBULAR CLUSTER METALLICITY SCALE FROM THE CA II TRIPLET II. RANKINGS, COMPARISONS, AND PUZZLES , 1997, astro-ph/9707068.
[74] S. Cassisi,et al. The ‘tip’ of the red giant branch as a distance indicator: results from evolutionary models , 1997, astro-ph/9703186.
[75] A. Renzini,et al. Tests of evolutionary sequences using color-magnitude diagrams of globular clusters , 1988 .
[76] Wendy L. Freedman,et al. The tip of the Red Giant Branch as a Distance Indicator for Resolved Galaxies: II. Computer Simulations , 1995 .
[77] L. Aller,et al. The chemical composition of the sun. , 1976, Science.
[78] P. Stetson,et al. THE AGE OF THE GALACTIC GLOBULAR CLUSTER SYSTEM , 1996 .
[79] S. Cassisi,et al. A critical investigation on the discrepancy between the observational and the theoretical red giant luminosity function ‘bump’ , 1997, astro-ph/9702029.
[80] A. Renzini,et al. The development of the red giant branch. I - Theoretical evolutionary sequences , 1989 .
[81] Paolo Ventura,et al. Predictions for Self-Pollution in Globular Cluster Stars , 2001 .
[82] P. Eggleton. The Evolution of Partially Degenerate Helium Cores , 1968 .
[83] M. Fujimoto,et al. The Origin of Extremely Metal-poor Carbon Stars and the Search for Population III , 2000, The Astrophysical journal.
[84] V. Castellani,et al. Stellar evolution as a probe of neutrino properties , 1993 .
[85] R. P. Kraft. ABUNDANCE DIFFERENCES AMONG GLOBULAR CLUSTER GIANTS: PRIMORDIAL VS. EVOLUTIONARY SCENARIOS , 1994 .
[86] Tod R. Lauer,et al. Detection of the Tip of the Red Giant Branch in NGC 3379 (M105) in the Leo I Group Using the Hubble Space Telescope , 1997 .
[87] William A. Fowler,et al. Thermonuclear Reaction Rates, III , 1967 .
[88] M. Bolte,et al. Globular Cluster Giant Branch Luminosity Functions: “Extra Stars” and “Deep Mixing” , 2000 .
[89] V. Smith,et al. Carbon isotopic abundances in giant stars in the CN-bimodal globular clusters NGC 6752 and M4 , 1991 .
[90] W. H. Kegel,et al. Problems in stellar atmospheres and envelopes , 1975 .
[91] R. J. Dickens,et al. An Analysis of G-Band Strengths in NGC 6397 and M55 Red Giants , 1990 .
[92] A. Weiss,et al. Evolution of Low-Mass Metal-Free Stars including Effects of Diffusion and External Pollution , 1999, astro-ph/9911270.
[93] V. Smith,et al. Star-to-Star Abundance Variations among Bright Giants in the Mildly Metal-poor Globular Cluster M4 , 1999, astro-ph/9905370.
[94] C. Charbonnel. A Consistent Explanation for [TSUP]12[/TSUP]C/[TSUP]13[/TSUP]C, [TSUP]7[/TSUP]Li, and [TSUP]3[/TSUP]He Anomalies in Red Giant Stars , 1995 .
[95] I. Iben,et al. Single star evolution I. Massive stars and early evolution of low and intermediate mass stars , 1984 .
[96] H. Hayashi,et al. Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes , 1996 .
[97] D. Alves,et al. The Age-dependent Luminosities of the Red Giant Branch Bump, Asymptotic Giant Branch Bump, and Horizontal Branch Red Clump , 1998, astro-ph/9808253.
[98] C. Proffitt,et al. Implications of helium diffusion for globular cluster isochrones and luminosity functions , 1991 .
[99] G. Piotto,et al. Star Counts across the Red Giant Branch Bump and Below , 2001 .
[100] I. Mazzitelli,et al. Stellar Turbulent Convection: A New Model and Applications , 1991 .
[101] C. Deliyannis,et al. Keck HIRES Spectroscopy of M92 Subgiants: Surprising Abundances near the Turnoff , 1998 .
[102] S. Cassisi,et al. A new analysis of the red giant branch ‘tip’ distance scale and the value of the Hubble constant , 1998, astro-ph/9803103.
[103] Achim Weiss,et al. Stellar Structure and Evolution , 1990 .
[104] P. Montegriffo,et al. A New Infrared Array Photometric Survey of Galactic Globular Clusters: A Detailed Study of the Red Giant Branch Sequence as a Step toward the Global Testing of Stellar Models , 1999, astro-ph/9912265.
[105] Kiyoshi Katō,et al. A Model of Deep Mixing in Globular Cluster Red Giants , 1999 .
[106] M. Catelán,et al. The Helium-Core Mass at the Helium Flash in Low-Mass Red Giant Stars: Observations and Theory , 1995, astro-ph/9509062.
[107] K. K. Gilroy. Carbon isotope ratios and lithium abundances in open cluster giants , 1989 .
[108] W. Hubbard,et al. THERMAL CONDUCTION BY ELECTRONS IN STELLAR MATTER. , 1969 .
[109] G. Wasserburg,et al. Deep Circulation in Red Giant Stars: A Solution to the Carbon and Oxygen Isotope Puzzles? , 1995 .
[110] C. Sneden,et al. SODIUM-OXYGEN ABUNDANCE ANTICORRELATIONS AND DEEP MIXING SCENARIOS FOR GLOBULAR CLUSTER GIANTS , 1993 .
[111] Forrest J. Rogers,et al. Updated Opal Opacities , 1996 .
[112] V. Castellani,et al. Mass loss in globular cluster red giants : an evolutionary investigation , 1993 .
[113] A. Weiss,et al. An updated theoretical scenario for globular cluster stars , 1997, astro-ph/9707180.
[114] D. Sugimoto. Helium Flash in Less Massive Stars , 1964 .
[115] I. Iben,et al. Helium flashes and hydrogen mixing in low-mass population III stars , 1990 .
[116] N. Suntzeff,et al. Carbon and nitrogen abundances in giant stars of the metal-poor globular cluster M92 , 1982 .
[117] B. Freytag,et al. Stellar Envelope Convection Calibrated by Radiation Hydrodynamics Simulations: Influence on Globular Cluster Isochrones , 1999, astro-ph/9901074.
[118] M. Fukugita,et al. A Study of the B−V Color-Temperature Relation , 1999, astro-ph/9904299.
[119] France.,et al. A standard stellar library for evolutionary synthesis - II. The M dwarf extension , 1997, astro-ph/9710350.
[120] M. Shetrone. Al, Mg and Eu Abundances in Globular Cluster Giants. I. Tests of Deep Mixing , 1996 .
[121] C. Sneden,et al. Proton Capture Chains in Glubular Cluster Stars. I. Evidence for Deep Mixing Based on Sodium and Magnesium Abundances in M13 Giants , 1996 .
[122] Michael J. West,et al. The globular cluster system of the Galaxy. III: measurements of radial velocity and metallicity for 60 clusters and a compilation of metallicities for 121 clusters , 1984 .
[123] A. Renzini,et al. The development of the red giant branch. II - Astrophysical properties , 1990 .
[124] A. Renzini,et al. Four experiments on thermal instabilities in stellar envelopes , 1994 .
[125] N. Suntzeff. Carbon and nitrogen abundances in the giant stars of the globular clusters M3 and M13 , 1981 .
[126] D. Alexander,et al. Models for Old, Metal-poor Stars with Enhanced α-Element Abundances. I. Evolutionary Tracks and ZAHB Loci; Observational Constraints , 2000 .
[127] R. Hoffman,et al. OBSERVATIONAL CONSTRAINTS ON THE ORIGIN OF THE ALUMINUM ENHANCEMENTS AND MAGNESIUM DEPLETIONS IN BRIGHT M13 GIANTS , 1997 .
[128] Models for Old, Metal-poor Stars with Enhanced α-Element Abundances. III. Isochrones and Isochrone Population Functions , 2001, astro-ph/0102480.
[129] B. Ricci,et al. Stellar evolution and large extra dimensions , 2000, astro-ph/0002182.
[130] Oscar Straniero,et al. The alpha -enhanced Isochrones and Their Impact on the FITS to the Galactic Globular Cluster System , 1993 .
[131] David R. Alexander,et al. Low-Temperature Rosseland Opacities , 1975 .
[132] John P. Cox,et al. Principles of stellar structure , 1968 .
[133] Bruce W. Carney,et al. THE CONSTANCY OF [ALPHA/FE] IN GLOBULAR CLUSTERS OF DIFFERING [FE/H] AND AGE , 1996 .
[134] I. Iben. Low-Mass Red Giants , 1968 .
[135] D. VandenBerg,et al. The prediction of stellar effective temperatures from the mixing-length theory of convection , 1990 .
[136] Johns Hopkins University,et al. Improved Color-Temperature Relations and Bolometric Corrections for Cool Stars , 1999, astro-ph/9911367.
[137] A. Chieffi,et al. The Luminosity Function of M3 , 1999, astro-ph/9905193.
[138] W. Fowler,et al. Thermonuclear reaction rates V , 1988 .
[139] The Origin of Extreme Horizontal Branch Stars , 1995, astro-ph/9511017.
[140] R. G. Gratton,et al. Abundances for globular cluster giants: I. homogeneous metallicities for 24 clusters , 1996, astro-ph/9607078.
[141] Garching,et al. A Contribution of 26Al to the O-Al Anticorrelation in Globular Cluster Red Giants , 2001, astro-ph/0107190.
[142] M. Dworetsky,et al. Peculiar versus Normal Phenomena in A-type and Related Stars , 1993 .
[143] J. Norris,et al. The Sodium/Aluminum--Oxygen Anticorrelation in omega Centauri and Other Clusters , 1995 .
[144] H. Schlattl,et al. On the Helium Flash in Low-Mass Population III Red Giant Stars , 2001, astro-ph/0105410.