Radiatively efficient accreting black holes in the hard state: the case study of H1743-322 H1743-322: radio/X-ray correlation (2011)
Attributed to:
High Energy Astrophysics at Southampton
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1111/j.1365-2966.2011.18433.x
Publication URI: http://dx.doi.org/10.1111/j.1365-2966.2011.18433.x
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1