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Table 2

Hot B subdwarf stars with masses determined by light curve modeling and spectroscopy in binary systems.

Name Log g Teff M1 Nature Eclipses References
(cm s-2) (K) (M)

KPD 0422+5421 5.565  ±  0.009 25 000  ±  1500 0.511  ±  0.049a sdB+WD yes Orosz & Wade (1999)
PG 1241 − 084 5.63  ±  0.03 28 490  ±  210 0.48  ±  0.09 sdB+dM yes Wood & Saffer (1999)
5.60  ±  0.12 28 490  ±  210 0.485  ±  0.013a Lee et al. (2009)
HS 0705+6700 5.40  ±  0.10 28 800  ±  900 0.48 sdB+dM yes Drechsel et al. (2001)
HS 2333+3927 5.70  ±  0.10 36 500  ±  1000 0.38 sdB+dM no Heber et al. (2005)
NSVS 14256825 5.50  ±  0.02 35 000  ±  5000 0.46 sdB+dM yes Wils et al. (2007)
KPD 1930+2752 5.61  ±  0.06 35 200  ±  500 0.485  ±  0.035a sdB+WD yes Geier et al. (2007)
PG 1336 − 018 5.74  ±  0.05 31 300  ±  300 0.389  ±  0.005 sdB+dM yes Vuckovic et al. (2007)
5.77  ±  0.06 31 300  ±  300 0.466  ±  0.006
5.79  ±  0.07 31 300  ±  300 0.530  ±  0.007
2M 1533+3759 5.57  ±  0.07 29 230  ±  125 0.376  ±  0.055a sdB+dM yes For et al. (2010)
2M 1938+4603 5.425  ±  0.009 29 565  ±  105 0.48  ±  0.03a sdB+dM yes Østensen et al. (2010)
KPD 1946+4340 5.452  ±  0.006 34 500  ±  400 0.47  ±  0.03a sdB+WD yes Bloemen et al. (2011)
AA Dor 5.46  ±  0.05 42 000  ±  1000 0.471  ±  0.005a sdB+dM? no Klepp & Rauch (2011)

Notes. 

(a)

Masses retained for our analysis.

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