Discovery of a new black hole transient within 100" (400 pc) of M31*

Abstract

We identified a new X-ray transient CXOM31 004252.457+411631.17 (T13) in M31 during a 2013 June Chandra observation. This system is particularly exciting because it is located within 100" of M31*; it is thought that this region of the bulge is sufficiently dense to form X-ray binaries dynamicaly, but only systems with black hole accretors and/or short periods are expected to survive. A follow-up XMM-Newton observation yielded a soft spectrum, well described by a 0.39+/-0.02 keV disk blackbody; applying this model to the Chandra observation yielded an observed 0.3--10 keV luminosity peak of 6.2+/-0.6 E+37 erg/s (4.7 E+36 erg/s in the 2.0--10 keV band). Observing with HST/ACS did not reveal an optical counterpart, but allowed us to place an upper limit of B >26.9, corresponding to an absolute V band magnitude >2.0. From the 2--10 keV luminosity and absolute V magnitude, we estimate an orbital period $<$5 h from an empirical relation. Fitting a disk blackbody + blackbody model allows us to reject a neutron star accretor at a 14 sigma level.

Accepted for publication in ApJ. 4 pages, 4 figures. arXiv admin note: substantial text overlap with arXiv:1305.1302

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• Candidate isolated neutron stars in the 4XMM-DR10 catalog of X-ray sources
• Chandra, XMM-Newton and HST observations of a transient in M31 with a possible asymmetric, precessing disk