CORE
🇺🇦
make metadata, not war
Services
Services overview
Explore all CORE services
Access to raw data
API
Dataset
FastSync
Content discovery
Recommender
Discovery
OAI identifiers
OAI Resolver
Managing content
Dashboard
Bespoke contracts
Consultancy services
Support us
Support us
Membership
Sponsorship
Community governance
Advisory Board
Board of supporters
Research network
About
About us
Our mission
Team
Blog
FAQs
Contact us
Galactic population of black holes in detached binaries with low-mass stripped helium stars: The case of LB-1 (LS V+22 25)
Authors
Kolesnikov D.A.
Kuranov A.G.
Postnov K.A.
Yungelson L.R.
Publication date
1 January 2020
Publisher
Abstract
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We model the Galactic population of detached binaries that harbour black holes with 0.5-1.7 M companions - remnants of case B mass exchange that rapidly cross Hertzsprung gap after the termination of the Roche lobe overflow or as He-shell burning stars. Several such binaries can be currently present in the Galaxy. The range of MBH in them is about 4-10 M, and the orbital periods are tens to hundreds of days. The unique black hole binary LB-1 fits well into this extremely rare class of double stars
Similar works
Full text
Available Versions
Kazan Federal University Digital Repository
See this paper in CORE
Go to the repository landing page
Download from data provider
oai:dspace.kpfu.ru:net/162385
Last time updated on 03/05/2021