1998PASP..110..784H

Query : 1998PASP..110..784H

1998PASP..110..784H - Publ. Astron. Soc. Pac., 110, 784-793 (1998/July-0)

Time-resolved photometry and spectroscopy of the cataclysmic variable V592 Cassiopeiae.

HUBER M.E., HOWELL S.B., CIARDI D.R. and FRIED R.

Abstract (from CDS):

Over the past 10 years, the cataclysmic variable (CV) V592 Cassiopeiae (LS I 55 -8) has been monitored by one of the authors. We now present time-resolved optical and infrared photometry and optical spectroscopy of this nova-like binary. Analysis of these data provides the first orbital solution for this star. We find an orbital period near 0.114 days (2.7 hr), a system inclination of 28°, and a mass ratio (M2/M1) of 0.19. V592 Cas appears to be a nova-like cataclysmic variable with a massive white dwarf primary and lies inside the CV period gap.

Abstract Copyright: ∼

Journal keyword(s): Stars: Novae, Cataclysmic Variables - stars: individual (V592 Cassiopeiae) - stars: individual (LS I 55 -8 (read: LS I +55 8))

CDS comments: Table 2: comparison stars C(V), K(V), C(IR) and K(IR are not in SIMBAD, but C(V) = [HH95] V592 Cas -, and K(V) = [HH95] V592 Cas-14.

Simbad objects: 7

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Number of rows : 7
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 [HH95] V592 Cas-7 * 00 20 40.67 +55 41 47.0   14.091 13.497     ~ 2 0
2 V* V592 Cas CV* 00 20 52.2230598456 +55 42 16.235113356 12.07 12.86 12.79 12.783   OB 109 0
3 2MASS J00205373+5542192 * 00 20 53.7418134168 +55 42 19.222896564   14.817 13.445     ~ 5 0
4 V* WX Ari CV* 02 47 36.2217912312 +10 35 37.723782948   15.8       ~ 66 0
5 EGB 4 CV* 06 29 33.9600353880 +71 04 36.394613580   13.29 13.27 13.04   ~ 170 0
6 V* BK Lyn CV* 09 20 11.2020621696 +33 56 42.356468364   13.97 13.99 14.72   ~ 125 1
7 HD 203856 * 21 23 35.5297279464 +40 01 07.023676800   7.33 7.21     A0V 85 0

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