Two newly identified eclipsing binaries in open cluster NGC 3532

We present light curve analyses of two newly identified detached eclipsing binaries, HD 96609 and HD 303734, in the region of the richly populated open cluster NGC 3532. HD 96609 is composed of two main sequence stars (B9-A0V + A2V) with masses and radii of $M_{1}=2.66\pm0.02$$M_{\odot}\(, \)M_{2}=1...

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Veröffentlicht in:	arXiv.org 2021-10
1. Verfasser:	Özdarcan, Orkun
Format:	Artikel
Sprache:	eng
Schlagworte:	Age Clusters Light curve Main sequence stars Physics - Astrophysics of Galaxies Physics - Solar and Stellar Astrophysics
Online-Zugang:	Volltext
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