X-ray binaries in M51 I: catalog and statistics

Abstract

We used archival data from the \emph{Chandra X-ray Observatory} (\emph{Chandra}) and the \emph{Hubble Space Telescope}, to identify 334 candidate X-ray binary (XRB) systems and their potential optical counterparts in the interacting galaxy pair NGC 5194/5195 (M51). We present the catalog and data analysis of X-ray and optical properties for those sources, from the deep $892$ ks \emph{Chandra} observations, along with the magnitudes of candidate optical sources as measured in the $8.16$ ks \emph{HST} observations. The X-ray luminosity function of the X-ray sources above a few times $10^{36}\mathrm{erg}{\mathrm{s}}^{-1}$ follows a power law $N(>L_{X,b})\propto L_{X,b}^{1-\alpha }$ with $\alpha =1.65\pm 0.03$. Aproximately 80\% of sources are variable over a 30 day window. Nearly half of the X-ray sources (173/334) have an optical counterparts within $0{\mbox{$.\!\!^{\prime\prime}$}}5$.

10 pages; accepted for publication in ApJ; matches accepted version

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Cited by in corpus (1)

• The Missing Link Between Black Holes in High-Mass X-ray Binaries and Gravitational-Wave Sources: Observational Selection Effects