A ultraluminous X-ray source associated with a cloud collision in M 99

Monthly Notices of the Royal Astronomical Society

Volumn 372, Issue 4, 2006, Pages 1531-1539

  Soria, Roberte ^a,b   Wong, Diane Sonya ^c  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Black hole physics; Galaxies: individual: NGC 4254; Radio lines: galaxies; X rays: binaries; X rays: galaxies

Indexed keywords

BLACK HOLES; ELECTRON SOURCES; GALAXIES; GAMMA RAYS; GRAVITATION; LUMINANCE; X RAY APPARATUS;

BLACK HOLE PHYSICS; GALAXIES: INDIVIDUAL: NGC 4254; RADIO LINES:GALAXIES; SPIRAL PATTERN; STAR FORMATION RATES; TIDAL INTERACTIONS; X-RAY LUMINOSITY; X-RAY SOURCES; X-RAYS: BINARIES; X-RAYS: GALAXIES;

STARS;

EID: 33750438404     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10981.x     Document Type: Article

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