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Photometric Analysis of Variable Stars in NGC 299

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.

preprint2013arXivOpen access
R. J. SandersI. SerrajP. C. SchmidtkeA. Udalski
astro-ph.SR
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Open access4 authors1 topic
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R. J. SandersI. SerrajP. C. SchmidtkeA. Udalski

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