Wind from the black-hole accretion disk driving a molecular outflow in an active galaxy

F. Tombesi (), M. Meléndez, S. Veilleux, J. N. Reeves, E. González-Alfonso and C. S. Reynolds
Additional contact information
F. Tombesi: X-ray Astrophysics Laboratory, NASA/Goddard Space Flight Center
M. Meléndez: University of Maryland, College Park
S. Veilleux: University of Maryland, College Park
J. N. Reeves: Astrophysics Group, School of Physical and Geographical Sciences, Keele University, Keele, Staffordshire ST5 5BG, UK
E. González-Alfonso: Universidad de Alcalá, Campus Universitario, E-28871 Alcalá de Henares, Madrid, Spain
C. S. Reynolds: University of Maryland, College Park

Nature, 2015, vol. 519, issue 7544, 436-438

Abstract: Observations of an ultrafast accretion-disk wind in the X-ray spectrum of a nearby ultraluminous infrared galaxy support the theory that such winds affect the evolution of supermassive black holes and their host galaxies.

Date: 2015
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/nature14261 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:519:y:2015:i:7544:d:10.1038_nature14261

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

DOI: 10.1038/nature14261

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 ().