An Unusual Spectral State of an Ultra-luminous Very Soft X-ray Source during Outburst

Details An Unusual Spectral State of an Ultra-luminous Very Soft X-ray Source during Outburst An Unusual Spectral State of an Ultra-luminous Very Soft X-ray Source during Outburst

2005-09-19

arxiv.org/abs/astro-ph/0509567v1

Astrophys.J.632:L107-L110,2005

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, accepted for publication in ApJL

Scientific paper

10.1086/498020

We report the results of Chandra and XMM-Newton observations of a new outburst of an ultra-luminous X-ray source in M101. During a Chandra monitoring observation of M101, M101 ULX-1 was found to be in outburst in 2004 December, the second outburst in 2004. The peak bolometric luminosity is about 3e40 erg/s (7e39 erg/s in 0.3-7 keV). The outburst spectra are very soft and can generally be fitted with a blackbody model with temperatures of 40-80 eV, similar to supersoft X-ray sources in the Milky Way and in the Magellanic Clouds. In one Chandra observation, the source spectrum appears to be harder with a temperature of 150 eV. Such a spectral state is rarely seen in M101 ULX-1 and no X-ray source in the Milky Way shows this kind of spectrum. However, such an unusual spectral state very likely belongs to a new class of X-ray sources, quasisoft X-ray sources, recently discovered in nearby galaxies. M101 ULX-1 returned to supersoft state in a subsequent XMM-Newton observation. Based on the two outbursts in 2004, the extremely high luminosity (L_bol=1e40-1e41 erg/s), very soft X-ray spectra (kT=40-150 eV), transient behavior, and state transition provide strong evidence that M101 ULX-1 harbors an intermediate-mass black hole.

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