PARADIGM THAT ULTRALUMINOUS X-RAY SOURCES AS A CLASS REPRESENT ACCRETING INTERMEDIATE-MASS BLACK HOLES

Record Type
Journal Articles
Full Title
PARADIGM THAT ULTRALUMINOUS X-RAY SOURCES AS A CLASS REPRESENT ACCRETING INTERMEDIATE-MASS BLACK HOLES
Author(s)
Berghea C, Weaver K, Colbert E, Roberts T
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2008 Nov 1
DOI
10.1086/591722
ISSN
0004-637X
Volume
687
Issue
1
Page Count
17
First Page
471
Last Page
487
Keyword(s)
Astronomy & Astrophysics, accretion, accretion disks, galaxies: general, surveys, X-rays: binaries, XMM-NEWTON OBSERVATIONS, POINT-SOURCE POPULATION, HIGH-RESOLUTION CAMERA, NEARBY SPIRAL GALAXIES, SOURCE NGC-5204 X-1, CHANDRA OBSERVATIONS, STARBURST GALAXY, SUPERNOVA REMNANT, ANTENNAE GALAXIES, CIRCINUS GALAXY
Citation
Berghea C, Weaver K, Colbert E, Roberts T. PARADIGM THAT ULTRALUMINOUS X-RAY SOURCES AS A CLASS REPRESENT ACCRETING INTERMEDIATE-MASS BLACK HOLES. ASTROPHYS J. 2008;687 (1):471-487.
Conditions of Use
  • Author can archive pre-print (i.e., pre-refereeing)
  • Author can archive post-print (i.e., final draft post-refereeing)
  • On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository.
  • Publisher's version/PDF may be used on any website or authors' institutional repository
  • Publisher copyright and source must be acknowledged
  • Must link to publisher version
  • Publisher's version/PDF may be used
  • Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article – a "non-exclusive licence to distribute"
  • Publisher last contacted on 10/02/2016

More usage information may be available at SHERPA/RoMEO