The Ultraluminous X-ray Source NGC 1313 X-2 (MS 0317.7-6647) and its Environment
arXiv:astro-ph/0310739 · doi:10.1086/381541
Abstract
We present new optical and {\it Chandra} observations of the field containing the ultraluminous X-ray source NGC 1313 X-2. On an ESO 3.6 m image, the {\it Chandra} error box embraces a point-like object and excludes a previously proposed optical counterpart. The resulting X-ray/optical flux ratio of NGC 1313 X-2 is . The value of , the X-ray variability history and the spectral distribution derived from a re-analysis of the {\it ROSAT}, {\it ASCA} and {\it XMM} data indicate a luminous X-ray binary in NGC 1313 as a likely explanation for NGC 1313 X-2. If the X-ray soft component observed in the {\it XMM} EPIC spectrum originates from an accretion disk, the inferred mass of the compact remnant is , making it an intermediate mass black hole. The derived optical luminosity () is consistent with that of a companion. The properties of the environment of NGC 1313 X-2 are briefly discussed.
arXiv comment12 pages, 6 figures; submitted to The Astrophysical Journal
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