Strong disk winds traced throughout outbursts in black-hole X-ray binaries

B. E. Tetarenko (), J.-P. Lasota, C. O. Heinke, G. Dubus and G. R. Sivakoff
Additional contact information
B. E. Tetarenko: University of Alberta
J.-P. Lasota: Institut d’Astrophysique de Paris, CNRS et Sorbonne Universités
C. O. Heinke: University of Alberta
G. Dubus: Université Grenoble Alpes, CNRS, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG)
G. R. Sivakoff: University of Alberta

Nature, 2018, vol. 554, issue 7690, 69-72

Abstract: Analysis of the light curves of outbursts in black-hole X-ray binaries suggests that throughout the accretion process mass is lost from the accretion disks through strong, magnetically driven disk winds.

Date: 2018
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/nature25159 Abstract (text/html)
Access to the full text of the articles in this series is restricted.

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:554:y:2018:i:7690:d:10.1038_nature25159

Ordering information: This journal article can be ordered from
https://www.nature.com/

DOI: 10.1038/nature25159

Access Statistics for this article

Nature is currently edited by Magdalena Skipper

More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().