Application of the Thermal Wind Model to Absorption Features in the Black Hole X-ray Binary H 1743-322 (2019)
Attributed to:
Durham Astronomy Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1906.02469
Publication URI: https://arxiv.org/abs/1906.02469
Type: Other