Peak Luminosities of the Hard States of GX 339-4: Implications for the Accretion Geometry, Disk Mass, and Black Hole Mass (2007)

First Author: Yu W

Attributed to: High Energy Astrophysics at Southampton funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1086/518733

Publication URI: http://dx.doi.org/10.1086/518733

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2