Document Detail


A black hole nova obscured by an inner disk torus.
MedLine Citation:
PMID:  23449588     Owner:  NLM     Status:  In-Process    
Abstract/OtherAbstract:
Stellar-mass black holes (BHs) are mostly found in x-ray transients, a subclass of x-ray binaries that exhibit violent outbursts. None of the 50 galactic BHs known show eclipses, which is surprising for a random distribution of inclinations. Swift J1357.2-093313 is a very faint x-ray transient detected in 2011. On the basis of spectroscopic evidence, we show that it contains a BH in a 2.8-hour orbital period. Further, high-time-resolution optical light curves display profound dips without x-ray counterparts. The observed properties are best explained by the presence of an obscuring toroidal structure moving outward in the inner disk, seen at very high inclination. This observational feature should play a key role in models of inner accretion flows and jet collimation mechanisms in stellar-mass BHs.
Authors:
J M Corral-Santana; J Casares; T Muñoz-Darias; P Rodríguez-Gil; T Shahbaz; M A P Torres; C Zurita; A A Tyndall
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Publication Detail:
Type:  Journal Article; Research Support, Non-U.S. Gov't    
Journal Detail:
Title:  Science (New York, N.Y.)     Volume:  339     ISSN:  1095-9203     ISO Abbreviation:  Science     Publication Date:  2013 Mar 
Date Detail:
Created Date:  2013-03-01     Completed Date:  -     Revised Date:  -    
Medline Journal Info:
Nlm Unique ID:  0404511     Medline TA:  Science     Country:  United States    
Other Details:
Languages:  eng     Pagination:  1048-51     Citation Subset:  IM    
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, S/C de Tenerife, Spain. jcorral@iac.es
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