Astronomy and Astrophysics – Astronomy
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.3501k&link_type=abstract
American Astronomical Society Meeting 210, #35.01; Bulletin of the American Astronomical Society, Vol. 39, p.148
Astronomy and Astrophysics
Astronomy
Scientific paper
We report the discovery of a recurrent ultraluminous X-ray source (ULX) in the starburst galaxy M82. From a series of Chandra observations, we found an ULX (Lx 1e40 erg/s) that was active for about 100 days in late 1999. The source turned off in 2000 January for about 50 days and has been active since then, indicating at least a factor of 50 in brightness variation. During its active state, the source luminosity varies between 7e39 erg/s and 1e40 erg/s and shows unusual spectral changes. The X-ray spectra are best fit with a power-law with photon index of 1.2-1.7. By comparing with IR images taken with HST/NICMOS, the ULX is found to be located within a young star cluster. Radio imaging indicates that it is associated with an extended radio source. We suggest that the ULX is likely a >100 solar mass intermediate-mass black hole in the low/hard state. In addition to the transient, we also found a very luminous (Lx 2e39 erg/s) X-ray emitting supernova remnant and a highly absorbed hard ULX within 3 arcsec of the transient. Finally, we will discuss the diverse properties of ULXs in M82.
Hsieh P.
Kong Albert K.
Mak D. S.
Pun C. S.
Yang Yadong
No associations
LandOfFree
A Recurrent Ultraluminous X-ray Transient In M82: Another Intermediate-mass Black Hole? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Recurrent Ultraluminous X-ray Transient In M82: Another Intermediate-mass Black Hole?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Recurrent Ultraluminous X-ray Transient In M82: Another Intermediate-mass Black Hole? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1030237