Journal ArticleOPEN ACCESS

Donor Stars in Black Hole X‐Ray Binaries

  • Kalogera V
The Astrophysical Journal (1999) 521(2) 723-734
DOI: 10.1086/307562
52Citations
Citations of this article
6Readers
Mendeley users who have this article in their library.

Abstract

We study theoretically the formation of black hole (BH) X-ray binaries. Consistency of the models with the observed relative numbers of systems with low-mass ( 1) are required, implying that energy sources other than orbital contraction must be invoked to eject the envelope; and (3) the mass-loss fraction in helium star winds is limited to

Cite

CITATION STYLE

APA

Kalogera, V. (1999). Donor Stars in Black Hole X‐Ray Binaries. The Astrophysical Journal, 521(2), 723–734. https://doi.org/10.1086/307562

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free