Helium-rich subluminous stars

Fundamental Data

Star alpha(2000)delta(2000) m_B Ref
29517-49 00 03 32 -16 43 59 1
29503-9 00 04 30 1
HS0025+344 00 27 47.9+34 40 26 15.4 2
PHL 780 00 18 36.6+15 21 55 16.2 3
PG0135+242 01 38 08.5+24 30 14 15.1 3
PG0216+246 02 19 44.3+24 47 28 15.9 3
PG0245+182 02 48 07.3+18 26 08 15.8 3
22968-19 03 09 48 -56 23 57 1
HS0315+339 03 18 42.3+34 05 55 16.5 2
22190-3 03 44 59 -16 52 39 14.9 1
LB 1766 04 59 19.3-53 52 55 12.3 4
HS0836+620 08 40 44.1+61 47 52 14.8 2
PG0902+058 09 05 05.3+05 33 01 14.1 3
PG0914-037 09 17 16.1-03 53 50 16.4 3
PG0950+158 09 53 17.1+15 33 40 15.9 3
PG0959-083 10 01 33.3-08 42 44 16.1 3
HS1000+471 10 03 24.2+46 49 45 17.1 2
PG1127+019 11 30 03.8+01 37 34 13.0 3
%PG1144+005 11 46 35.6+00 12 29 15.0 3
TON 107 12 41 59.8+43 40 46 16.3 3
%PB 146 13 18 47.3+44 35 44 14.8 3
PG1413+114 14 15 49.1+11 12 12 15.6 3
PG1415+492 14 17 02.7+48 57 29 14.4 3
PG1437+727 14 37 30.7+72 28 44 13.6 3
PG1441+407 14 43 21.6+40 28 31 15.5 3
PG1526+440 15 28 02.4+43 50 17 15.7 3
PG1544+488 15 46 11.7+48 38 37 12.0 3
PG1553+464 15 54 26.9+46 17 00 16.0 3
PG1554+407 15 55 50.4+40 38 51 15.9 3
PG1559+222 16 01 13.8+22 05 48 14.5 3
PG1601+171 16 03 04.1+16 59 54 16.3 3
PG1616+413 16 17 38.8+41 12 52 16.4 3
PG1630+466 16 31 18.0+46 31 01 14.0 3
PG1648+315 16 50 22.8+31 27 49 16.0 3
PG1658+273 17 00 14.3+27 12 35 15.7 3
PG1715+273 17 17 03.2+27 16 37 16.2 3
HS1844+637 18 43 59.8+63 46 51 16.1 2
HS1909+656 19 08 43.8+65 39 06 17.0 2
22885-43 20 18 15 -38 34 01 1
22940-9 20 30 20 -59 50 49 14.1 1
LS IV-14 11620 57 39 -14 25 48 13.0 5
JL 87 21 48 37.9-76 20 45 11.9 6
22956-90 22 14 58 -63 41 46 1
22956-94 22 16 56 -64 31 50 1
22938-44 22 52 20 -63 15 52 1
PG2258+155 23 00 57.8+15 48 40 15.0 3
22893-20 23 08 30 -11 38 41 1
PG2322+214 23 24 27.2+21 38 52 12.9 3
29496-10 23 34 02 -28 51 37 1
PG2339+199 23 41 56.6+20 12 17 15.8 3

References

1. Beers T.C., Preston G.W., Shectman S.A., Doinidis S.P., Griffin K.E., 1992, AJ 103.1, 267.
2. Heber U., Dreizler D., Werner K., Engels D., Hagen H.-J. (these Proceedings).
3. Green R.F., Schmidt M., Liebert J., 1986, ApJS 61, 305.
4. Kilkenny D., Busse J., 1992, MNRAS 258, 57.
5. Viton M., Deleuil M., Tobin W., Prevot L., Bouchet P., 1991, A&A 242, 175.
6. Schulz H., Heber U., Wegner G., 1991, PASP 103, 435.