Evidence of an Intermediate-Mass Black Hole: Chandra and XMM-Newton Observations of the Ultraluminous Supersoft X-Ray Source in M101 during Its 2004 Outburst-Reference-Cited by-同舟云学术

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Evidence of an Intermediate-Mass Black Hole: Chandra and XMM-Newton Observations of the Ultraluminous Supersoft X-Ray Source in M101 during Its 2004 Outburst

Published:2004-11-04 Issue:1 Volume:617 Page:L49-L52
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Kong A. K. H.,Di Stefano R.,Yuan F.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference33 articles.

1. Super-Eddington Fluxes from Thin Accretion Disks?

2. Parameter estimation in astronomy through application of the likelihood ratio

3. XMM‐NewtonObservations of an Intermediate X‐Ray Object in NGC 2276

4. H I in the Galaxy

5. Luminous Supersoft X‐Ray Sources in External Galaxies

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3. On the Magnetic Fields, Beaming Fractions, and Fastness Parameters of Pulsating Ultraluminous X-Ray Sources;The Astrophysical Journal;2020-08-17

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