2000MNRAS.317..310H


Query : 2000MNRAS.317..310H

2000MNRAS.317..310H - Mon. Not. R. Astron. Soc., 317, 310-314 (2000/September-2)

Gravitational radiation from strongly magnetized white dwarfs.

HEYL J.S.

Abstract (from CDS):

The magnetic fields of white dwarfs distort their shape generating an anisotropic moment of inertia. A magnetized white dwarf that rotates obliquely relative to the symmetry axis has a mass quadrupole moment that varies in time, so it will emit gravitational radiation. The Laser Interferometer Space Antenna (LISA) mission may be able to detect the gravitational waves from two nearby, rapidly rotating white dwarfs.

Abstract Copyright: 2000, Royal Astronomical Society

Journal keyword(s): gravitation - binaries: close - stars: magnetic fields - novae, cataclysmic variables - white dwarfs

CDS comments: Table 1: RE J0317+853 misprint for J0317-853, PG 1015+14 misprint for 1015+014

Simbad objects: 32

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Number of rows : 32
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Feige 7 WD* 00 43 45.9806246832 -10 00 25.016051736   14.49       DBAP3 114 0
2 V* BL Hyi CV* 01 41 00.3996430344 -67 53 27.470100660       15.340   DC: 221 0
3 V* WW Hor CV* 02 36 11.4433563560 -52 19 13.934884433           ~ 81 0
4 V* XY Ari CV* 02 56 08.19048 +19 26 34.1844           ~ 167 1
5 V* CL Oct WD* 03 17 15.8468594712 -85 32 25.558244556   13.78 13.66 15.19   DAP 180 1
6 LB 9802 WD* 03 17 19.1282833488 -85 32 31.288377552   13.78 13.66 14.43   DA 141 1
7 V* GK Per No* 03 31 12.0098863320 +43 54 15.469951212   14.139 13.090 12.589   K1IV 986 0
8 V* UZ For CV* 03 35 28.6518733656 -25 44 21.768755424           M4.5 279 0
9 V* V471 Tau SB* 03 50 24.9666549840 +17 14 47.430910716   10.258 9.373   8.393 K2V+DA 697 0
10 V* V1062 Tau CV* 05 02 27.4778229096 +24 45 23.157957240   17.159 16.717 16.319   ~ 85 0
11 V* TV Col CV* 05 29 25.5292422792 -32 49 03.900212364   14.219 13.846 14.181   K2V 362 0
12 V* TW Pic CV* 05 34 50.5861498896 -58 01 40.765120788 13.84 14.83 15.10     ~ 107 2
13 V* BG CMi CV* 07 31 29.0079060264 +09 56 23.030740248   14.5       ~ 246 0
14 V* PQ Gem CV* 07 51 17.3280306912 +14 44 23.874868716   14.415 14.162 13.945   ~ 237 0
15 V* VV Pup CV* 08 15 06.8009599464 -19 03 17.765706024     13.90     M7V 413 0
16 V* VZ Pyx CV* 08 59 19.8388698120 -24 28 55.257493908     14.08     ~ 69 0
17 PG 1015+014 ** 10 18 05.0427157728 +01 11 23.527902156   16.33 16.3     DA+M 82 0
18 Ton 527 WD* 10 33 49.1967544416 +23 09 16.254781992   15.3 15.73     DAP2 120 0
19 V* ST LMi CV* 11 05 39.7664319408 +25 06 28.746723096   16.832 16.524 15.639   DAH+M 228 0
20 V* DO Dra CV* 11 43 38.4921265896 +71 41 20.559036192       13.747   DQ 233 1
21 V* EX Hya CV* 12 52 24.2222471899 -29 14 55.999766523   13.505 13.491 13.549   M5-6V 730 0
22 V* V834 Cen CV* 14 09 07.2863511816 -45 17 16.023776676       15.301   M6.5 333 0
23 PG 1550+191 CV* 15 52 47.1968971224 +18 56 28.844471472   16.4 15.46 17.0   M6.5Ve 202 0
24 V* DQ Her CV* 18 07 30.2510391864 +45 51 32.564791872   14.605 14.443 14.800   M3+Ve 1048 1
25 V* V533 Her No* 18 14 20.4844831200 +41 51 22.069747872   15.000 15.032 15.274   ~ 265 0
26 V* AM Her CV* 18 16 13.2546725104 +49 52 04.759613537   15.124 14.808 13.525   M4.5-5Ve 1009 2
27 V* CW Sgr Mi* 19 06 47.8237466352 -11 54 35.037589248           ~ 6 0
28 V* WZ Sge CV* 20 07 36.5037622512 +17 42 14.733254952   15.30 15.20 10.817   D 982 0
29 V* AE Aqr CV* 20 40 09.1598959176 -00 52 15.055595220   12.46 10.40   10.191 K3-5IV/V 705 0
30 V* V1500 Cyg No* 21 11 36.5809818696 +48 09 01.952490204           ~ 820 0
31 V* FO Aqr CV* 22 17 55.3796835600 -08 21 03.754995948   13.533 13.445 13.414   ~ 378 0
32 V* AO Psc CV* 22 55 17.9860863984 -03 10 39.981831564           ~ 327 0

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