Photometric Analysis of Variable Stars in NGC 299
classification
🌌 astro-ph.SR
keywords
starsvariableanalysisanalyzedbinariesclusterclusterseclipsing
read the original 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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.