Photometric Analysis of Variable Stars in NGC 299
Solar and Stellar Astrophysics
2013-04-23 v5
Abstract
We have analyzed OGLE-III photometry for stars in the SMC cluster NGC 299. Two eclipsing binaries and one intrinsic variable (most likely a Be star) are identified. Unlike other young SMC clusters, no low-amplitude pulsating variables are present.
Cite
@article{arxiv.1302.6943,
title = {Photometric Analysis of Variable Stars in NGC 299},
author = {R. J. Sanders and I. Serraj and P. C. Schmidtke and A. Udalski},
journal= {arXiv preprint arXiv:1302.6943},
year = {2013}
}
Comments
Draft Version April 15th, 2013 accepted for publication in IBVS on April 19, 2013. 8 pages, 1 table, 4 figures