parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
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L. Girardi | B. Salasnich | A. Bressan | P. Marigo | S. Rubele | C. Cero | A. Nanni | Claudia Dal Cero
[1] P. Bogdanovich,et al. Atomic Data and Nuclear Data Tables , 2013 .
[2] A. Dotter,et al. MODELS FOR METAL-POOR STARS WITH ENHANCED ABUNDANCES OF C, N, O, Ne, Na, Mg, Si, S, Ca, AND Ti, IN TURN, AT CONSTANT HELIUM AND IRON ABUNDANCES , 2012, 1206.1820.
[3] A. Korn,et al. ATOMIC DIFFUSION AND MIXING IN OLD STARS. III. ANALYSIS OF NGC 6397 STARS UNDER NEW CONSTRAINTS , 2012, 1204.5600.
[4] S. Degl'Innocenti,et al. The Pisa Stellar Evolution Data Base for low-mass stars , 2012, 1202.4864.
[5] N. Mowlavi,et al. Stellar mass and age determinations - I. Grids of stellar models from Z = 0.006 to 0.04 and M = 0.5 to 3.5 M⊙ , 2012, 1201.3628.
[6] Joana M. Oliveira,et al. The VMC survey - IV. The LMC star formation history and disk geometry from four VMC tiles , 2011, 1110.5852.
[7] M. Pinsonneault,et al. Asteroseismology of old open clusters with Kepler: direct estimate of the integrated red giant branch mass-loss in NGC 6791 and 6819 , 2011, 1109.4376.
[8] N. Panagia,et al. PHOTOMETRIC DETERMINATION OF THE MASS ACCRETION RATES OF PRE-MAIN-SEQUENCE STARS. II. NGC 346 IN THE SMALL MAGELLANIC CLOUD , 2011, 1104.4494.
[9] J. Christensen-Dalsgaard,et al. A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology , 2011, 1102.0235.
[10] A. Pietrinferni,et al. The magnitude difference between the main sequence turn off and the red giant branch bump in Galactic globular clusters , 2010, 1012.0419.
[11] Ryan M. Ferguson,et al. THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS , 2010, The Astrophysical Journal Supplement Series.
[12] T. Lebzelter,et al. The pulsation of AGB stars in the Magellanic Cloud clusters NGC 1978 and 419 , 2010, 1006.3121.
[13] L. Casagrande,et al. Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion , 2010, 1005.2944.
[14] A. Weiss,et al. ON USING THE COLOR–MAGNITUDE DIAGRAM MORPHOLOGY OF M67 TO TEST SOLAR ABUNDANCES , 2010, 1004.3308.
[15] Bernd Freytag,et al. Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere , 2010, 1003.1190.
[16] P. Morel,et al. Survival of a convective core in low-mass solar-like pulsator HD 203608 , 2010, 1002.3461.
[17] M. Nonino,et al. ON THE ΔVbumpHB PARAMETER IN GLOBULAR CLUSTERS , 2010, 1002.2074.
[18] L. Girardi,et al. Scaled solar tracks and isochrones in a large region of the Z-Y plane. II. From 2.5 to 20 solar masses , 2009, 0911.2419.
[19] J. Ferguson,et al. NEW SOLAR COMPOSITION: THE PROBLEM WITH SOLAR MODELS REVISITED , 2009, 0909.2668.
[20] M. Asplund,et al. The chemical composition of the Sun , 2009, 0909.0948.
[21] Austria,et al. Low-temperature gas opacity. ÆSOPUS: a versatile and quick computational tool , 2009, 0907.3248.
[22] W. Chaplin,et al. FRESH INSIGHTS ON THE STRUCTURE OF THE SOLAR CORE , 2009, 0905.0651.
[23] I. Kamp,et al. The solar photospheric nitrogen abundance - Analysis of atomic transitions with 3D and 1D model atmospheres , 2009, 0903.3406.
[24] L. Girardi,et al. Discovery of two distinct red clumps in NGC 419: a rare snapshot of a cluster at the onset of degeneracy , 2009, 0901.0773.
[25] P. Bonifacio,et al. The photospheric solar oxygen project. I. Abundance analysis of atomic lines and influence of atmosp , 2008, 0805.4398.
[26] Darko Jevremovic,et al. The Dartmouth Stellar Evolution Database , 2008, 0804.4473.
[27] L. Girardi,et al. Revised Bolometric Corrections and Interstellar Extinction Coefficients for the ACS and WFPC2 Photometric Systems , 2008, 0804.0498.
[28] P. Bonifacio,et al. The solar photospheric abundance of hafnium and thorium: Results from CO5BOLD 3D hydrodynamic model atmospheres , 2008, 0803.3585.
[29] Astronomy Department,et al. Scaled solar tracks and isochrones in a large region of the Z-Y plane I. From the ZAMS to the TP-A , 2008, 0803.1460.
[30] Gepi,et al. The solar photospheric abundance of europium Results from CO5BOLD 3D hydrodynamical model atmospheres , 2008, 0803.0863.
[31] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[32] Belgium,et al. Evolution of asymptotic giant branch stars. II. Optical to far-infrared isochrones with improved TP- , 2007, 0711.4922.
[33] S. Nozawa,et al. The Second Born Corrections to the Electrical and Thermal Conductivities of Dense Matter in the Liquid Metal Phase , 2007, 0708.2967.
[34] P. Bonifacio,et al. The solar photospheric abundance of phosphorus : results from CO5BOLD 3D model atmospheres , 2007, 0708.1607.
[35] J. Ferguson,et al. A Constraint on Z☉ from Fits of Isochrones to the Color-Magnitude Diagram of M67 , 2007, 0708.1172.
[36] E. Caffau,et al. The forbidden 1082 nm line of sulphur: - the photospheric abundance of sulphur in the Sun and 3D effects , 2007, astro-ph/0703423.
[37] -INAF,et al. Evolution of asymptotic giant branch stars. I. Updated synthetic TP-AGB models and their basic calibration , 2007, astro-ph/0703139.
[38] P. Aguer,et al. Experimental determination of the O17(p,α)N14 and O17(p,γ)F18 reaction rates , 2007 .
[39] R. Bohlin. HST Stellar Standards with 1% Accuracy in Absolute Flux , 2006, astro-ph/0608715.
[40] C. Rossi-Alvarez,et al. S-factor of 14N(p,γ)15O at astrophysical energies⋆ , 2005, nucl-ex/0509005.
[41] The Isolde Collaboration,et al. Revised rates for the stellar triple-α process from measurement of 12C nuclear resonances , 2005, Nature.
[42] P. Stetson,et al. On the Old Open Clusters M67 and NGC 188: Convective Core Overshooting, Color‐Temperature Relations, Distances, and Ages , 2004 .
[43] C. Iliadis,et al. Investigation of the Na-23(p, gamma) Mg-24 and Na-23(p, alpha) Ne-20 reactions via (He-3, d) spectroscopy , 2004 .
[44] A. Coc,et al. Compilation and R-matrix analysis of Big Bang nuclear reaction rates , 2004, astro-ph/0407101.
[45] S. Cassisi,et al. A Large Stellar Evolution Database for Population Synthesis Studies. I. Scaled Solar Models and Isochrones , 2004, astro-ph/0405193.
[46] H. M. Antia,et al. Constraining Solar Abundances Using Helioseismology , 2004, astro-ph/0403485.
[47] J. Richer,et al. Models for Solar Abundance Stars with Gravitational Settling and Radiative Accelerations: Application to M67 and NGC 188 , 2004, astro-ph/0402544.
[48] E. Sandquist. A high relative precision colour-magnitude diagram of M67 , 2003, astro-ph/0308547.
[49] H. Leiste,et al. Stellar He burning of18O:A measurement of low-energy resonances and their astrophysical implications , 2003 .
[50] P. Mohr,et al. The $^{15}$N($\bm\alpha$,$\bm\gamma$)$^{19}$F reaction and nucleosynthesis of $^{19}$F , 2002, nucl-ex/0211031.
[51] L. Girardi,et al. Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets , 2002, astro-ph/0205080.
[52] W. H. Fenton,et al. Heavy-Element Diffusion in Metal-poor Stars , 2001, astro-ph/0108119.
[53] W. J. Thompson,et al. Proton-induced Thermonuclear Reaction Rates for A = 20–40 Nuclei , 2001 .
[54] F. Allard,et al. The Limiting Effects of Dust in Brown Dwarf Model Atmospheres , 2001, astro-ph/0104256.
[55] L. Girardi,et al. Zero-metallicity stars I. Evolution at constant mass , 2001, astro-ph/0102253.
[56] S. Lucatello,et al. The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters , 2000, astro-ph/0012457.
[57] H. Leiste,et al. Low-energy resonances in 14N(a,?)18F and their astrophysical implications , 2000 .
[58] J. Richer,et al. The Evolution of AmFm Stars, Abundance Anomalies, and Turbulent Transport , 2000 .
[59] 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.
[60] M. Pinsonneault,et al. How Much Do Helioseismological Inferences Depend on the Assumed Reference Model? , 1999, astro-ph/9909247.
[61] P. Aguer,et al. A compilation of charged-particle induced thermonuclear reaction rates , 1999 .
[62] F. Rogers,et al. Consistent Solar Evolution Model Including Diffusion and Radiative Acceleration Effects , 1998 .
[63] N. Grevesse,et al. Standard Solar Composition , 1998 .
[64] Sarbani Basu,et al. Seismic measurement of the depth of the solar convection zone , 1997 .
[65] Forrest J. Rogers,et al. Updated Opal Opacities , 1996 .
[66] A. Weiss,et al. Standard and Nonstandard Plasma Neutrino Emission Revisited , 1993, astro-ph/9309014.
[67] L. Marschall,et al. CCD photometry of the old open cluster M67 , 1993 .
[68] A. Loeb,et al. Element Diffusion in the Solar Interior , 1993, astro-ph/9304005.
[69] M. Pinsonneault,et al. Standard solar model , 1992 .
[70] A. Bressan,et al. New Developments in Understanding the HR Diagram , 1992 .
[71] W. Fowler,et al. Thermonuclear reaction rates V , 1988 .
[72] N. Itoh,et al. Neutrino Energy Loss in Stellar Interiors , 1985 .
[73] N. Itoh,et al. Neutrino-pair bremsstrahlung in dense stars. I: Liquid metal case , 1983 .
[74] M. S. Cooper,et al. Screening factors for nuclear reactions. I. General theory , 1973 .
[75] H. E. DeWitt,et al. Screening Factors for Nuclear Reactions. 11. Intermediate Screen-Ing and Astrophysical Applications , 1973 .
[76] A. Cameron,et al. Abundances of the elements in the solar system , 1973 .
[77] E. Böhm-Vitense,et al. Über die Wasserstoffkonvektionszone in Sternen verschiedener Effektivtemperaturen und Leuchtkräfte. Mit 5 Textabbildungen , 1958 .