Spectral analyses of the nearest persistent ultraluminous X-Ray source M 33 X-8

Publications of the Astronomical Society of Japan

Volumn 61, Issue 6, 2009, Pages 1287-1291

  Weng, Shan Shan ^a   Wang, Jun Xian ^b   Gu, Wei Min ^a   Lu, Ju Fu ^a  

^a XIAMEN UNIVERSITY   (China)

^b UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

Author keywords

Accretion; Accretion disks ; Black hole physics ; Individual (m 33 x 8) ; X rays; X rays binaries ; X rays stars

Indexed keywords

BLACK HOLES; ELECTRON SOURCES; GRAVITATION; SPECTRUM ANALYSIS; STARS; X RAY APPARATUS;

ACCRETION; ACCRETION DISCS; ACCRETION DISK -; BLACK HOLE PHYSIC -; BLACK HOLE PHYSICS; INDIVIDUAL (M 33 X-8) -; INDIVIDUAL:M 33; X-RAY BINARY-; X-RAY:STARS; X-RAYS: BINARIES;

SIGNAL TO NOISE RATIO;

EID: 76649102152     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/61.6.1287     Document Type: Article

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