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Table 3:

Parameters of some typical hot subdwarfs and their progenitors.
$M_{\rm 1i}$ / $M_{\rm f}($type) $q_{\rm i}$ $P_{\rm i}$ / $P_{\rm f}$ $M_{\rm env}$ $t_{\rm age}$
($M_{\odot }$)   (days) ($M_{\odot }$) (yrs)
conservative case:        
3.55/0.38(sdB) 1.1 1.5/151.1 0.02 $3.8\times 10^{8}$
3.55/0.56(sdB) 1.1 3.5/116.1 0.04 $0.9\times 10^{8}$
3.55/0.53(sdB) 4.0 3.5/11.5 0.04 $1.1\times 10^{8}$
5.01/0.54(sdB) 1.1 1.6/147.8 0.04 $1.0\times 10^{8}$
5.01/0.65(sdOB) 1.1 2.5/137.3 0.05 $0.6\times 10^{8}$
5.01/0.93(sdO) 1.1 15.7/317.2 0.09 $0.2\times 10^{8}$
5.01/1.01(sdOB) 1.1 31.3/483.8 0.12 $0.2\times 10^{8}$
5.01/1.06(sdB) 1.1 40.6/545.5 0.16 $0.1\times 10^{8}$
5.01/0.84(sdO) 4.0 5.1/13.1 0.08 $0.2\times 10^{8}$
5.01/0.91(sdO) 4.0 32.3/60.8 0.09 $0.2\times 10^{8}$
non-conservative case:        
3.55/0.33(sdB) 1.1 1.5/27.9 0.01 $7.9\times 10^{8}$
3.55/0.54(sdB) 1.1 3.5/29.4 0.04 $1.0\times 10^{8}$
3.55/0.53(sdB) 4.0 3.5/6.9 0.04 $1.1\times 10^{8}$
5.01/0.46(sdB) 1.1 1.6/27.2 0.03 $1.7\times 10^{8}$
5.01/0.61(sdOB) 1.1 2.5/29.0 0.05 $0.7\times 10^{8}$
5.01/0.91(sdO) 1.1 15.7/100.5 0.09 $0.2\times 10^{8}$
5.01/0.98(sdOB) 1.1 41.6/483.2 0.12 $0.2\times 10^{8}$
5.01/1.00(sdB) 1.1 43.6/526.0 0.14 $0.1\times 10^{8}$
5.01/0.84(sdO) 4.0 5.1/9.1 0.08 $0.3\times 10^{8}$
5.01/0.91(sdO) 4.0 32.3/59.4 0.09 $0.2\times 10^{8}$
$M_{\rm 1i} =$ initial mass; $M_{\rm f} =$ the mass of hot subdwarfs; $q_{\rm i}=$ the mass ratio; $P_{\rm
i} =$ initial orbital period; $P_{\rm f} =$ orbital period of hot subdwarf binaries; $M_{\rm env} =$ the envelope mass of hot subdwarfs; $t_{\rm age} =$ the lifetime of a hot subdwarf. More parameters can be seen from Figs. 2, 3, and 6-9.

Source LaTeX | All tables | In the text

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