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Table 3:

Confirmed binary systems containing a low-mass white dwarf.

Name
$P_{\rm orb}$ (days) $M_{\rm WD}$ ($M_\odot$) Reference
NLTT 11748 0.2351 $0.167\pm0.005$ 1, 2
NS + WD
PSR B1855+09 12.3272 $0.258\pm0.020$ 3
PSR J0437-4715 5.7410 $0.254\pm0.018$ 4
PSR J0218+4232 2.0288 $0.275\pm0.105$ 5, 6
PSR J1909-3744 1.5334 $0.204\pm 0.002$ 7
PSR J1911-5958A 0.8371 $0.175\pm0.010$ 8, 9
PSR J1012+5307 0.6047 $0.16\pm0.02$ 10, 11, 12
PSR J1738+0333 0.3548 $0.20\pm 0.05$ 13
PSR J0751+1807 0.2631 $0.191\pm0.015$ 14
WD + WD
LP400-22 1.010 $0.190\pm0.004$ 15
SDSS J0822+2753 0.244 $0.17\pm 0.01$ 16
SDSS J1257+5428 0.1898 $0.20\pm 0.05$ 17
SDSS J0849+0445 0.079 $0.17\pm 0.01$ 16
SDSS J1436+5010 0.0458 $0.23\pm 0.01$ 16
SDSS J1053+5200 0.0426 $0.22\pm 0.01$ 16
Progenitors
HD 188112 0.6066 $0.24\pm0.10$ 18
SDSS J1023+0038 0.1981 $0.2\pm 0.05$ 19, 20

References. (1) This work; (2) Kawka & Vennes (2009); (3) Kaspi et al. (1994); (4) Verbiest et al. (2008); (5) Navarro et al. (1995); (6) Bassa et al. (2003); (7) Jacoby et al. (2005); (8) Corongiu et al. (2006); (9) Bassa et al. (2006); (10) Webb et al. (2004); (11) van Kerkwijk et al. (1996); (12) Callanan et al. (1998); (13) Freire et al. (2008); (14) Nice et al. (2005); (15) Vennes et al. (2009); (16) Kilic et al. (2010); (17) Marsh et al. (2010); (18) Heber et al. (2003); (19) Archibald et al. (2009); (20) Wang et al. (2009).


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