
\magnification=900

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\def\ie{{\rm i.e.\ }}
\def\etal{{\rm et al.\ }}
\def\chem#1#2{$\rm{}^{#2}\kern-0.8pt#1$}
\def\mass#1{$\rm #1\,M_{\odot}$}
\def\lum#1{$\rm #1\,L_{\odot}$}
\def\rad#1{$\rm #1\,R_{\odot}$}
\def\teff{$\rm T_{\rm e \mkern -1.8mu f \mkern -1.8mu f}\,$}
\def\tim#1#2{$\rm #1 \, 10^{#2}$}

{
\catcode`\@=\active \def@{\hphantom{0}}
\noindent {\bf Tables 1.}\ 
           Evolution of some key features for the calculated PMS models.
           From the left to the right, we give the star age (in yr), the
           total luminosity ($\rm L_*$/\lum{}), the total radius ($\rm
           R_*$/\rad{}), the effective temperature (\teff), the energetic
           contribution of the nuclear reactions in units of $\rm L_*$
           ($\rm L_{nuc}$; in \%), the gravitational energy release ($> 0$) or
           absorption ($< 0$) in units of $\rm L_*$ ($\rm L_{grav}$; in \%),
           the mass of the radiative core ($\rm M_{core}$, in \mass{}),
           the temperature at the base of the convective envelope ($\rm T_b$,
           equal to the central temperature during the completely convective
           phase), and the surface \chem{Li}{6}, \chem{Li}{7} and \chem{Be}{9}
           abundances (relative to their initial value).  Each table is
           labelled by the total mass $\rm M_*$ and the metallicity Z of the
           concerned star.  When non-standard physics is used (\ie not that
           presented in Sect. 2), it is explicitely indicated.  The number
           of selected lines for each model is chosen in order to allow
           accurate enough interpolations in the various quantities.
\bigskip
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\noalign{\smallskip\hrule\medskip}
 $\rm \log t$ & $\rm L_*$/\lum{} & $\rm R_*$/\rad{} & \teff &%
 $\rm L_{nuc}$/$\rm L_*$ & $\rm L_{grav}$/$\rm L_*$ & $\rm M_{core}$/\mass{} &%
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\noalign{\smallskip\hrule\medskip}
 $\rm \log t$ & $\rm L_*$/\lum{} & $\rm R_*$/\rad{} & \teff &%
 $\rm L_{nuc}$/$\rm L_*$ & $\rm L_{grav}$/$\rm L_*$ & $\rm M_{core}$/\mass{} &%
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 $\rm \log t$ & $\rm L_*$/\lum{} & $\rm R_*$/\rad{} & \teff &%
 $\rm L_{nuc}$/$\rm L_*$ & $\rm L_{grav}$/$\rm L_*$ & $\rm M_{core}$/\mass{} &%
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\noalign{\smallskip\hrule\medskip}
 $\rm \log t$ & $\rm L_*$/\lum{} & $\rm R_*$/\rad{} & \teff &%
 $\rm L_{nuc}$/$\rm L_*$ & $\rm L_{grav}$/$\rm L_*$ & $\rm M_{core}$/\mass{} &%
 $\rm \log T_b$ & \chem{Li}{6}/\chem{Li}{6}$|_0$ &%
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 $\rm \log t$ & $\rm L_*$/\lum{} & $\rm R_*$/\rad{} & \teff &%
 $\rm L_{nuc}$/$\rm L_*$ & $\rm L_{grav}$/$\rm L_*$ & $\rm M_{core}$/\mass{} &%
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 $\rm \log t$ & $\rm L_*$/\lum{} & $\rm R_*$/\rad{} & \teff &%
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\bye
