arXiv · 2201.07242
A Chandra Virgo cluster survey of spiral galaxies. I. Introduction to the survey and a new ULX sample
Abstract
We present an analysis of the ultraluminous X-ray source (ULX) population in 75 Virgo cluster late-type galaxies, including all those with a star formation rate >~ 1 M_{sun}/yr and a representative sample of the less star-forming ones. This study is based on 110 observations obtained over 20 years with the Chandra X-ray Observatory Advanced Camera for Imaging Spectroscopy. As part of a Large Chandra Program, new observations were obtained for 52 of these 75 galaxies. The data are complete to a sensitivity of about 10^{39} erg/s, with a typical detection limit of about 3 x 10^{38} erg/s for the majority of the sources. The catalogue contains about 80 ULXs (0.3-10 keV luminosity >10^{39} erg/s), and provides their location, observed flux, de-absorbed luminosity, and (for the 25 most luminous ones) simple X-ray spectral properties. We discuss the ULX luminosity function in relation to the mass and star formation rate of the sample galaxies. We show that recent models of low-mass plus high-mass X-ray binary populations (scaling with stellar mass and star formation rate, respectively) are mostly consistent with our observational results. We tentatively identify the most luminous X-ray source in the sample (a source in IC 3322A with L_{X} ~ 6 x 10^{40} erg/s) as a recent supernova or its young remnant. The properties of the sample galaxies (morphologies, stellar masses, star formation rates, total X-ray luminosities from their point-source population) are also summarised.
Explore related subjects
Keep this discovery
Roberto Soria, Mari Kolehmainen, Alister W. Graham, Douglas A. Swartz, Mihoko Yukita, Christian Motch, Thomas H. Jarrett, James C. A. Miller-Jones, Richard M. Plotkin, Thomas J. Maccarone, Laura Ferrarese, Alexander Guest, Ariane Lançon. 2022-01-18. A Chandra Virgo cluster survey of spiral galaxies. I. Introduction to the survey and a new ULX sample. https://doi.org/10.1093/mnras/stac148
Cite the original work for its findings. Save a collection to share your selection of sources.