The eclipsing binary PG 1323-086A (GSC 05544-00493)
Document Type
Article
Publication Date
1-1-2010
Abstract
The star PG 1323-086A (GSC 05544-00493) is shown to be a short-period eclipsing binary system. Photometric elements for the system are computed and reveal that the stellar components are in a marginal degree of contact (f ∼ 8%) with a small temperature difference of about 700 K. During the study of the starfield, a nearby object, HE 1323-0830, was also discovered to be variable in light. This star has been cataloged as a candidate blue straggler and is most likely a pulsating variable. © 2009. The Astronomical Society of the Pacific. All rights reserved.
Publication Source (Journal or Book title)
Publications of the Astronomical Society of the Pacific
First Page
27
Last Page
34
Recommended Citation
Clem, J., & Landolt, A. (2010). The eclipsing binary PG 1323-086A (GSC 05544-00493). Publications of the Astronomical Society of the Pacific, 122 (887), 27-34. https://doi.org/10.1086/649852