Multiband study of NGC 7424 and its two newly discovered ultraluminous X-ray sources

Monthly Notices of the Royal Astronomical Society

Volumn 370, Issue 4, 2006, Pages 1666-1676

  Soria, R ^a,b   Kuncic, Z ^c   Broderick, J W ^c   Ryder, S D ^d  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c UNIVERSITY OF SYDNEY   (Australia)

^d ANGLO AUSTRALIAN OBSERVATORY   (Australia)

Author keywords

Black hole physics; Galaxies: individual: NGC 7424; Radio continuum: ISM; Supernova remnants; X rays: binaries

Indexed keywords

ELECTRON SOURCES; LUMINANCE; PULSARS; RADIO ASTRONOMY; SUPERNOVAE; X RAY APPARATUS;

BLACK HOLE PHYSICS; CHANDRA; GALAXIES: INDIVIDUALS; GALAXY: INDIVIDUAL: NGC 7424; MULTI BAND; RADIO CONTINUUM: ISM; RADIO SPECTRAL INDEX; SUPERNOVA REMNANTS; X-RAY SOURCES; X-RAYS: BINARIES;

GALAXIES;

EID: 33746838054     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10629.x     Document Type: Review

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