1995BaltA...4..413O

Query : 1995BaltA...4..413O

1995BaltA...4..413O - Baltic Astronomy, 4, 413-421 (1995/November-0)

The AM CVn trial: the case for superhumps.

O'DONOGHUE D.

Abstract (from CDS):

The AM CVn stars are hydrogen deficient stars which are explained by an interacting binary white dwarf model. In this model, a low mass white dwarf fills its Roche lobe and transfers He-rich material to another white dwarf via an accretion disk. This paper advances a superhump mechanism to explain the photometric oscillations seen in the light curves of these stars.

Abstract Copyright: ∼

Journal keyword(s): stars: cataclysmic variables - stars: individual: AM CVn

Simbad objects: 6

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Number of rows : 6
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 V* V1159 Ori CV* 05 28 59.5676204544 -03 33 52.282939068   14.321 14.203 15.317   ~ 152 0
2 V* AM CVn CV* 12 34 54.6231062664 +37 37 44.120620056   14.02 14.13 14.47   DBnnp 434 0
3 V* V803 Cen CV* 13 23 44.5389056832 -41 44 29.446810404   16.8 14.42     ~ 155 0
4 V* HP Lib CV* 15 35 53.0715009672 -14 13 12.215196048   13.55       Bpec 112 0
5 GD 358 WD* 16 47 18.3925183824 +32 28 32.862804384 12.511 13.530 13.653 13.752 13.852 DB2 364 0
6 V* TY PsA CV* 22 49 39.9054462120 -27 06 53.126335980   15.61 15.67 16.19   DA 105 0

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