Evolved Eclipsing Binaries and the Age of the Open Cluster NGC 752

Evolved Eclipsing Binaries and the Age of the Open Cluster NGC 752

We present analyses of improved photometric and spectroscopic observations for two detached eclipsing binaries at the turnoff of the open cluster NGC 752: the 1.01 days binary DS And and the 15.53 days BD +37 410. For DS And, we find M _1 = 1.692 ± 0.004 ± 0.010 M _⊙ , R _1 = 2.185 ± 0.004 ± 0.008 R...

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Detalles Bibliográficos
Autores principales: Eric L. Sandquist, Andrew J. Buckner, Matthew D. Shetrone, Samuel C. Barden, Catherine A. Pilachowski, Constantine P. Deliyannis, Dianne Harmer, Robert Mathieu, Søren Meibom, Søren Frandsen, Jerome A. Orosz
Formato: Artículo
Lenguaje:English
Publicado: IOP Publishing 2022-01-01
Colección:The Astronomical Journal
Materias:
Eclipsing binary stars
Spectroscopic binary stars
Open star clusters
Low mass stars
Stellar ages
Stellar physics
Acceso en línea:https://doi.org/10.3847/1538-3881/ac9c59

Internet

https://doi.org/10.3847/1538-3881/ac9c59

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