Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds

Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds

Massive stars (∼8–25 M _⊙ ) stripped of their hydrogen-rich envelopes via binary interaction are thought to be the main progenitors for merging neutron stars and stripped-envelope supernovae. We recently presented the discovery of the first set of such stripped stars in a companion paper. Here, we f...

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Dettagli Bibliografici
Autori principali: Y. Götberg, M. R. Drout, A. P. Ji, J. H. Groh, B. A. Ludwig, P. A. Crowther, N. Smith, A. de Koter, S. E. de Mink
Natura: Articolo
Lingua:English
Pubblicazione: IOP Publishing 2023-01-01
Serie:The Astrophysical Journal
Soggetti:
Binary stars
Close binary stars
Interacting binary stars
Early-type stars
Helium-rich stars
Helium burning
Accesso online:https://doi.org/10.3847/1538-4357/ace5a3

Accesso online

https://doi.org/10.3847/1538-4357/ace5a3

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