Lightcurve Analysis of Six Beta-Lyrae Type Variables
Abstract
We present light curve analysis of six variable stars: NSVS 5344676, V1071 Her, NSVS 5508151, NSVS 9064159, NSVS 9091101, and NSVS 3714875. These objects are selected from beta-Lyrae candidates published in a paper by Hoffman et al (2008). Light curves are generated using data collected at the Truman State Observatory in four filters: Johnson R, V, B, and IR/UV. We compare our classification to the ones presented by Hoffman et al. We conclude that the first object, previously classified only as a variable star, should be reclassified as an Algol-type variable. The second object may either be a beta-Lyrae variable or a W UMa variable. We confirm Hoffman et al's classification of the third object as a beta-Lyrae variable. Data collection and analysis on the remaining three objects is ongoing. In this poster, we present the light curves on these six objects and comment on their classification as beta-Lyrae, Algol, or W UMa -type variables.
- Publication:
-
American Astronomical Society Meeting Abstracts #225
- Pub Date:
- January 2015
- Bibcode:
- 2015AAS...22534303G