J/A+A/285/473 Low-mass stars (Forestini 1994)
Low-mass stars: pre-main sequence evolution and nucleosynthesis; Abundances
FORESTINI M.
<Astron. Astrophys. 285, 473 (1994)>
=1994A&A...285..473F 1994A&A...285..473F
ADC_Keywords: Stars, pre-main sequenc; Mass loss; Models, evolutionary;
Keywords: stars: pre-main sequence - stars: evolution of - nucleosynthesis -
stars: abundances
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1 78 554 Evolutionary sequences
table1.tex 80 1176 LaTex version of table1
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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1- 3 F3.1 solMass M Total mass
5- 10 F6.4 Sun Z Star metallicity
11 A1 --- n Note (1)
14- 18 F5.3 [yr] log(t) Star age
20- 24 F5.2 solLum L* Total luminosity
26- 30 F5.2 solRad R Total radius
32- 36 I5 K Teff Effective temperature
38- 42 F5.1 % Lnuc Energetic contribution of the nuclear reaction
in units of L*
44- 48 F5.1 % Lgrav Gravitational energy release (>0)
or absorption (<0) in units of L*
50- 54 F5.3 solMass Mcore Mass of the radiative core
56- 60 F5.3 [K] logTb Temperature at the base of the convective
envelope
62- 66 F5.3 --- 6Li Surface 6Li abundance
(relative to its initial value)
68- 72 F5.3 --- 7Li Surface 7Li abundance
(relative to its initial value)
74- 78 F5.3 --- 9Be Surface 9Be abundance
(relative to its initial value)
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Note (1):
a: with low-temperature radiative opacity tables of Alexander (1983)
b: with low- and high-temperature radiative opacity tables of
Alexander (1983) and Huebner et al. (1977), respectively
c: with the atmospheric temperature stratification given by the analytic
T(tau) relation of Henyey et al. (1985)
d: with the atmosphere integrated up to an optical depth tau = 0.001
e: with alpha = 2
f: with alpha = 1
g: with mass accretion from the beginning and during 2.5 10+6 yr, at a
rate of 10-7 Msun/yr
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(End) Patricia Bauer [CDS] 27-Jan-1994