Original by
Paul Bradley - HTML Enhanced by Travis Metcalfe
(DAV | DBV | DOV)
WD#: entry in White Dwarf Database |
VAR*: discovery paper in NASA ADS |
Periods: low-res light curve image
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TABLE 1: Names, Positions, and Magnitudes of the ZZ Ceti (DAV)
Stars |
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WD # | NAME | VAR * | a (2000.0) | d (2000.0) | Teff
| V MAG. | B MAG. | Amp. | Periods |
| | | | | ×103K | | | mags | seconds |
0104 -464 | BPM 30551 | AX Phe | 01 06 56 | -46 10.2 | 11.3 | 15.26 | 15.43
| 0.22 | 823 + others |
0133 -116 | R 548 | ZZ Cet | 01 36 10 | -11 20.7 | 12.0 | 14.16 | 14.33
| 0.012 | 213,274 |
0246 +326 | KUV 02464+3239 | ?? Tri | 02 49 28 | +32 51.2 | 11.3 | 15.8 | -
| 0.10 | 832+others |
0341 -459 * | BPM 31594 | VY Hor | 03 43 25 | -45 48.7 | 11.5 | 15.03 | 15.24
| 0.28 | 402,618,C,H |
0416 +272 | HL Tau 76 | V411 Tau | 04 18 59 | +27 18.4 | 11.4 | 15.20 | 15.40
| 0.28 | 494,625,746,C,H |
0417 +361 | G 38-29 | V468 Per | 04 20 18 | +36 16.6 | 11.2 | 15.59 | 15.79
| 0.22 | ~ 1000,C,H |
0455 +553 | G 191-16 | BR Cam | 04 59 28 | +55 25.3 | 11.4 | 15.98 | 16.1
| 0.3 | 510,600,710,893,C,H |
0507 +0435 | HS0507+0435 | V1396 Ori | 05 10 13 | +04 38.6 | 11.8 | 15.36 | 15.6
| 0.2 | 355,445,560,C,H |
0517 +307 | GD 66 | V361 Aur | 05 20 38 | +30 48.5 | 12.0 | 15.56 | 15.78
| 0.02 | 197,272,302,819,C |
0836 +404 | KUV 08368+4026 | DF Lyn | 08 40 08 | +40 15.1 | - | 15.55 | 15.77
| 0.03 | 495,618 |
0858 +363 | GD 99 | VW Lyn | 09 01 49 | +36 07.2 | 11.8 | 14.55 | 14.74
| 0.07 | 350,481,592 |
0921 +354 * | G117-B15A | RY LMi | 09 24 17 | +35 16.9 | 11.6 | 15.50 | 15.72
| 0.05 | 215,271,304C,H |
1137 +423 | KUV 11370+4222 | IZ UMa | 11 39 41 | +42 05.3 | - | 16.56 | 16.78
| 0.006 | 257+others |
1159 +803 | G255-2 | BT Cam | 12 01 48 | +80 05.0 | 11.4 | 16.04 | -
| 0.04 | 685,830 + others |
1236 -495 | BPM 37093 | V886 Cen | 12 38 48 | -49 49.0 | 11.7 | 13.96 | 14.14
| 0.004 | ~ 600 |
1307 +354 * | GD 154 | BG CVn | 13 09 58 | +35 09.5 | 11.2 | 15.33 | 15.51
| 0.10 | 403,1089,1186,C,H |
1350 +656 | G 238-53 | DU Dra | 13 52 12 | +65 24.9 | 11.9 | 15.51 | 15.7
| 0.02 | ~ 206 |
1401 -147 | EC 14012-1446 | IU Vir | 14 03 57 | -15 01.1 | - | 15.67 | 15.50 | 0.30 | 610,724 + others |
1422 +095 * | GD 165 | CX Boo | 14 24 40 | +09 17.3 | 12.0 | 14.32 | 14.46
| 0.10 | 114,120,192,250,C |
1425 -811 * | L 19-2 | MY Aps | 14 32 18 | -81 20.1 | 12.1 | 13.75 | 14.00
| 0.03 | 113,118,143,192,350 |
1541 +650 | PG 1541+650 | KX Dra | 15 41 44 | +64 53.9 | 12.0 | - | 15.7
| 0.045 | 562,686, 757 |
1559 +369 | R 808 | TY CrB | 16 01 21 | +36 47.0 | 11.2 | 14.36 | 14.53
| 0.15 | 833,complex,C,H |
1647 +591 * | G 226-29 | DN Dra | 16 48 26 | +59 03.5 | 12.5 | 12.24 | 12.40
| 0.006 | 109 |
1714 -547 | BPM 24754 | V876 Ara | 17 18 54 | -54 47.1 | 12.9 | 15.60 | 15.87
| 0.07 | ~ 1100 |
1855 +338 | G 207-9 | V470 Lyr | 18 57 30 | +33 57.2 | 12.0 | 14.62 | 14.81
| 0.06 | 259,292,557,739,C |
1935 +276 * | G 185-32 | PY Vul | 19 37 13 | +27 43.3 | 12.1 | 12.97 | 13.15
| 0.02 | 141,215,C,H |
1950 +250 | GD 385 | PT Vul | 19 52 28 | +25 09.3 | 11.7 | 15.12 | 15.32
| 0.05 | 256,C |
2254 +126 | GD 244 | ?? Peg | 22 56 46 | +12 52.9 | 11.7 | - | 16.0
(pg)
| 0.04 | 203,256,295,307,C |
2303 +242 * | PG 2303+242 | KR Peg | 23 06 16 | +24 32.0 | 11.5
| 15.50 | 15.58(pg)
| 0.2 | 394,483,540,611,936,C,H |
2326 +049 * | G 29-38 | ZZ Psc | 23 28 49 | +05 15.0 | 11.8 | 13.03 | 13.17
| 0.27 | 284,615,820,C,H |
2348 -244 | EC 23487-2424 | HW Aqr | 23 51 22 | -24 08.2 | - | 15.33 | 15.52
| 0.24 | ~ 800-1000, complex |
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NOTES: A ``*'' indicates multi-site campaign coverage on this object.
Effective temperature reference is Bergeron et al. 1995, ApJ, 449, 258.
A ``C'' in the period column stands for combination frequencies,
and an ``H'' means harmonics are present.
TABLE 3: Names, Positions, and Magnitudes of the DBV Stars |
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WD # | NAME | VAR * | a (2000.0) | d (2000.0) | Teff | V MAG. | B MAG. | Amp. | Periods |
| | | | | ×(103)K | | | (mags) | (seconds) |
0513 +260 | KUV 05134+2605 | V1063 Tau | 05 16 28 | +26 08.6 | 23.3 | 16.3
| -
| 0.10 | 400, complex |
0954 +342 | CBS 114 | SW LMi | 09 57 50 | +33 59.7 | 23.3
| 17(pg) | -
| 0.30 | 650, complex |
1115 +158 * | PG 1115+158 | DT Leo | 11 18 23 | +15 33.5 | 21.8 | -
| 16.12(pg)
| 0.06 | 1000, complex |
1351 +489 * | PG 1351+489 | EM UMa | 13 53 10 | +48 40.4 | 22.6 | -
| 16.38(pg)
| 0.05 | 489+harmonics |
1456 +103 | PG 1456+103 | CW Boo | 14 58 33 | +10 08.3 | 22.4 | -
| 15.89(pg)
| 0.10 | 420-860, complex |
1645 +325 * | GD 358 | V777 Her | 16 47 19 | +32 28.5 | 24.7±0.3 | 13.65
| 13.54
| 0.10 | 700, complex |
1654 +160 | PG 1654+160 | V824 Her | 16 56 58 | +15 56.4 | 24.3 | -
| 16.15(pg)
| 0.10 | 150-850, complex |
2006 -523 * | EC 20058-5234 | QU Tel | 20 09 40 | -52 25.4 | 27.1 | 15.54 | | 0.07 | 134,195,204,257,281 |
2246 +120 | PG 2246+121 | ?? Peg | 22 48 44 | +12 20.0 | 23.2 | 16.73
| 16.23(pg)
| 0.05 | 256,286,330 |
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NOTE:
Temperatures are from:
Beauchamp, A., et al. 1999, ApJ, 516, 887. I am using the trace hydrogen
model atmosphere results from their Table 1.
A ``*'' indicates multi-site campaign coverage on this object.
TABLE 5: Names, Positions, and Magnitudes of the PG1159 (DOV)
Stars |
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