J/A+AS/109/441 Stellar models until He burning - I. (Claret, 1995)
Stellar models for a wide range of initial chemical compositions until helium
burning I. From X=0.60 to X=0.80 for Z=0.02
Claret A.
<Astron. Astrophys. Suppl. Ser. 109, 441 (1995)>
=1995A&AS..109..441C 1995A&AS..109..441C (SIMBAD/NED Reference)
ADC_Keywords: Models, evolutionary
Keywords: stars: binaries: general - evolution - interiors -
fundamental parameters - abundance
Abstract:
New grids of stellar evolutionary models are presented for a wide
range of initial hydrogen content around the solar composition. These
compositions are (X, Z) = (0.80, 0.02), (0.70, 0.02) and (0.60, 0.02).
Recent OPAL opacities with LS coupling and Grevesse composition were
adopted, and Alexander's tables were used for lower temperatures. We
consider models with core overshooting with αov=0.20, and
mixing length parameter l/Hp=1.52 that seems to represent well
double-lined eclipsing binary stars. Mass loss during the main
sequence and in the red giant phase were taken into account. The
nuclear network treats 14 isotopes and optionally the lithium burning
to study its depletion in less massive models during pre main sequence
evolution. The mass range covered goes from 1 up to 40M☉ and
the more massive models were followed until helium burning.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
tables 106 2193 Grids of stellar evolutionary models
--------------------------------------------------------------------------------
See also:
J/A+AS/114/549 : Stellar models until He burning - II. (Claret+, 1995)
J/A+AS/125/439 : Stellar models until He burning - III. (Claret+, 1997)
J/A+AS/133/123 : Stellar models until He burning - IV. (Claret+ 1998)
Byte-by-byte Description of file: tables
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 7 F7.4 [solMass] logM ]-0.23/1.6] Initial mass of the model
9- 12 F4.2 --- X [0.6/0.8] X initial composition (H)
14- 17 F4.2 --- Z [0.02] Z initial composition
20 I1 --- Overshoot [0/1] without (0) or with (1) overshooting
23- 34 E12.6 yr Age Age of models
37- 43 F7.4 [solLum] log(L) Total luminosity
46- 52 F7.4 [cm/s2] log(g) Surface gravity
56- 61 F6.4 [K] log(Teff) Effective temperature
64- 70 F7.4 --- log(k2) Apsidal motion constant (j=2)
73- 79 F7.4 --- log(k3) Apsidal motion constant (j=3)
82- 88 F7.4 --- log(k4) Apsidal motion constant (j=4)
90- 97 F8.4 --- alpha alpha = -E_p x R/GM^2
101-106 F6.4 ---- beta Fractional gyration radius
--------------------------------------------------------------------------------
Historical Notes:
* 03-Oct-1994: Received at CDS
* 27-Mar-1995: the caption of original tables 3 and 4 were interchanged
(Antonio Claret dos Santos );
the correction has been reported in "tables".
See also:
J/A+AS/114/549 : Paper II (From X=0.63 to X=0.80, for Z=0.01)
(End) Patricia Bauer [CDS] 27-Mar-1995