SIMBAD references

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

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:1998PASP..110..784H and select 'bookmark this link' or equivalent in the popup menu