The Stellar Content of the Young Open Cluster Berkeley 50 (IC 1310)

We observed the Galactic open cluster Berkeley 50 in order to determine its stellar content, distance, and age. We obtained UBV photometry of 1145 stars in a 12.′3 × 12.′3 field, and used Gaia proper motions and parallaxes to identify 64 members, of which we obtained spectra of the 17 brightest memb...

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Bibliografiska uppgifter
Huvudupphovsmän: Meghan Speckert, Philip Massey, Brian A. Skiff
Materialtyp: Artikel
Språk:English
Publicerad: IOP Publishing 2024-01-01
Serie:The Astronomical Journal
Ämnen:
Länkar:https://doi.org/10.3847/1538-3881/ad3de2