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...

Deskribapen osoa

Xehetasun bibliografikoak

Egile Nagusiak:	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
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2023-01-01
Saila:	The Astrophysical Journal
Gaiak:	Binary stars Close binary stars Interacting binary stars Early-type stars Helium-rich stars Helium burning
Sarrera elektronikoa:	https://doi.org/10.3847/1538-4357/ace5a3
Etiketak:	Etiketa erantsi Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!