SIMBAD references

2012IBVS.6038....1S - IAU Inform. Bull. Var. Stars, 6038, 1 (2012/October-0)

Final classification of the bright variable star WW CMa.

SZABADOS L.

Abstract (from CDS):

Following the discovery of its brightness variability, the bright (<V> = 9.2m) variable star WW CMa was classified as an RR Lyrae type, then a Cepheid type, and during a half century an unstudied variable star with rapid light changes. The ASAS photometric data clearly indicate its eclipsing binary nature with an orbital period of 2.5163489 days.

Abstract Copyright: ∼

Journal keyword(s): eclipsing binary, photometry, period change

Simbad objects: 1

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2012IBVS.6038....1S and select 'bookmark this link' or equivalent in the popup menu