The Statistical Properties of Galaxies Containing Ulxs

We present a statistical analysis of the properties of galaxies containing ultraluminous X-ray objects (ULXs). Our primary goal is to establish the fraction of galaxies containing a ULX as a function of ULX luminosity. Our sample is based on ROSAT HRI observations of galaxies. We find that ∼ 12% of galaxies contain at least one ULX with LX > 10 39 erg sand ∼ 1% of galaxies contain at least one ULX with LX > 10 40 erg s. These ULX frequencies are lower limits since ROSAT HRI observation would miss absorbed ULXs (i.e., with NH & 10 21 cm) and those within ∼ 10” of the nucleus (due to the positional error circle of the ROSAT HRI). The Hubble type distribution of galaxies with a ULX differs significantly from the distribution of types for nearby RC3 galaxies, but does not differ significantly from the galaxy type distribution of galaxies observed by the HRI in general. We find no increase in the mean FIR luminosity or FIR / K band luminosity ratio for galaxies with a ULX relative to galaxies observed by the HRI in general, however this result is also most likely biased by the soft bandpass of the HRI and the relatively low number of high SFR galaxies observed by the HRI with enough sensitivity to detect a ULX.