The Ultraluminous X-ray Source NGC 1313 X-2 (MS 0317.7-6647) and its Environment

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 $R=21.6$ point-like object and excludes a previously proposed optical counterpart. The resulting X-ray/optical flux ratio of NGC 1313 X-2 is $\sim 500$. The value of $f_X/f_{opt}$, 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 $\approx 100M_{\odot }$, making it an intermediate mass black hole. The derived optical luminosity ($L\approx 10^5{L}_{\odot }$) is consistent with that of a $\approx 15-20M_{\odot }$ companion. The properties of the environment of NGC 1313 X-2 are briefly discussed.

12 pages, 6 figures; submitted to The Astrophysical Journal