A Comparison of Intermediate-Mass Black Hole Candidate Ultraluminous X-Ray Sources and Stellar-Mass Black Holes-Reference-Cited by-同舟云学术

A Comparison of Intermediate-Mass Black Hole Candidate Ultraluminous X-Ray Sources and Stellar-Mass Black Holes

Published:2004-09-24 Issue:2 Volume:614 Page:L117-L120
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Miller J. M.,Fabian A. C.,Miller M. C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference36 articles.

1. Super-Eddington Fluxes from Thin Accretion Disks?

2. Probable intermediate-mass black holes in NGC 4559: XMM-Newton spectral and timing constraints

3. A Transition to a Low/Soft State in the Ultraluminous Compact X-Ray Source Holmberg II X-1

4. Fabbiano, G. & White, N. E. 2003, in Compact Stellar X-Ray Sources, ed. W. H. G. Lewin & M. van der Klis (Cambridge: Cambridge Univ. Press), in press (astro-ph/0307077)

5. ChandraObservations of “The Antennae” Galaxies (NGC 4038/9)

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