Abstract
We report the discovery of an X-ray source coincident with the nuclear star cluster at the dynamical center of the nearby late-type spiral galaxy NGC 2403. The X-ray luminosity of this source varies from below detection levels, ~1e35 erg/s in the 0.5-8.0 keV band, to 7e38 erg/s on timescales between observations of less than 2 months. The X-ray spectrum is well-fit by an accretion disk model consisting of multiple blackbody components and corresponding physically to a compact object mass of greater than approximately 5 solar masses. No pulsations nor aperiodic behavior is evident in its X-ray light curve on the short timescales of the individual observations. The X-ray properties of the source are more similar to those of the nuclear source X-8 in M33, believed to be a low-mass X-ray binary, then to those of the low-luminosity active galactic nucleus in NGC 4395. The brightness of the nuclear star cluster, M_I ~ -11.8 mag, is typical of clusters in late-type spirals but its effective radius, r_e \~ 12 pc, is several times larger than average indicating a relatively relaxed cluster and a low probability of a central massive object. The cluster has a mass 3e6 solar masses and an age of 1.4 Gyr estimating from its observed colors and brightness.
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