SIMBAD references

2016ApJ...827...46K - Astrophys. J., 827, 46-46 (2016/August-2)

A deep Chandra ACIS survey of M51.

KUNTZ K.D., LONG K.S. and KILGARD R.E.

Abstract (from CDS):

We have obtained a deep X-ray image of the nearby galaxy M51 using Chandra. Here we present the catalog of X-ray sources detected in these observations and provide an overview of the properties of the point-source population. We find 298 sources within the D_25 radii of NGC 5194/5, of which 20% are variable, a dozen are classical transients, and another half dozen are transient-like sources. The typical number of active ultraluminous X-ray sources in any given observation is ∼5, and only two of those sources persist in an ultraluminous state over the 12 yr of observations. Given reasonable assumptions about the supernova remnant population, the luminosity function is well described by a power law with an index between 1.55 and 1.7, only slightly shallower than that found for populations dominated by high-mass X-ray binaries (HMXBs), which suggests that the binary population in NGC 5194 is also dominated by HMXBs. The luminosity function of NGC 5195 is more consistent with a low-mass X-ray binary dominated population.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): galaxies: individual: M51 - galaxies: ISM - ISM: supernova remnants - X-rays: binaries - X-rays: general - X-rays: general

VizieR on-line data: <Available at CDS (J/ApJ/827/46): table2.dat table4.dat table5.dat table6.dat>

Nomenclature: Tables 4-5: [KLK2016] XNNN (Nos X1-X503).

Simbad objects: 514

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2023.01.31-23:35:38

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