4.6 Article

A catalog of candidate intermediate-luminosity X-ray objects

期刊

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
卷 143, 期 1, 页码 25-45

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IOP PUBLISHING LTD
DOI: 10.1086/342507

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catalogs; galaxies : general; X-rays : binaries; X-rays : galaxies

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ROSAT, and now Chandra, X-ray images allow studies of extranuclear X-ray point sources in galaxies other than our own. X-ray observations of normal galaxies with ROSAT and Chandra have revealed that off-nuclear, compact, intermediate-luminosity (L-X[2-10 keV]greater than or equal to10(39.0) ergs s(-1)) X-ray objects (IXOs, a.k.a. ULXs [ultraluminous X-ray sources]) are quite common. Here we present a catalog and finding charts for 87 IXOs in 54 galaxies, derived from all of the ROSAT HRI imaging data for galaxies with czless than or equal to5000 km s(-1) from the Third Reference Catalog of Bright Galaxies. We have defined the cutoff L-X for IXOs so that it is well above the Eddington luminosity of a 1.4 M-circle dot black hole (10(38.3) ergs s(-1)), so as not to confuse IXOs with normal black hole X-ray binaries. This catalog is intended to provide a baseline for follow-up work with Chandra and XMM-Newton, and with space- and ground-based survey work at wavelengths other than X-ray. We demonstrate that elliptical galaxies with IXOs have a larger number of IXOs per galaxy than non-elliptical galaxies with IXOs and note that they are not likely to be merely high-mass X-ray binaries with beamed X-ray emission, as may be the case for IXOs in starburst galaxies. Approximately half of the IXOs with multiple observations show X-ray variability, and many (19) of the IXOs have faint optical counterparts in DSS optical B-band images. Follow-up observations of these objects should be helpful in identifying their nature.

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