Abstract
Evidence is emerging that the luminous X-ray sources in the cores of globular clusters may often consist of, or perhaps even as a class be dominated by, ultracompact (P
Cite
CITATION STYLE
APA
Deutsch, E. W., Margon, B., & Anderson, S. F. (2000). Ultracompact X-Ray Binaries in Globular Clusters: Variability of the Optical Counterpart of X1832−330 in NGC 6652. The Astrophysical Journal, 530(1), L21–L24. https://doi.org/10.1086/312486
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free