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- W2233590947 abstract "Late type non-starburst galaxies have been shown to contain X-ray emitting objects, some being ultraluminous X-ray sources. We report on XMM-Newton observations of 11 nearby, late-type galaxies previously observed with the Hubble Space Telescope (HST) in order to find such objects. We found 18 X-ray sources in or near the optical extent of the galaxies, most being point-like. If associated with the corresponding galaxies, the source luminosities range from $2 times 10^{37}$ erg s$^{-1}$ to $6 times 10^{39}$ erg s$^{-1}$. We found one ultraluminous X-ray source, which is in the galaxy IC 5052, and one source coincident with the galaxy IC 4662 with a blackbody temperature of $0.166 pm 0.015$ keV that could be a quasi-soft source or a quiescent neutron star X-ray binary in the Milky Way. One X-ray source, XMMU J205206.0$-$691316, is extended and coincident with a galaxy cluster visible on an HST image. The X-ray spectrum of the cluster reveals a redshift of $z = 0.25 pm 0.02$ and a temperature of 3.6$pm$0.4 keV. The redshift was mainly determined by a cluster of Fe XXIV lines between the observed energy range $0.8-1.0$ keV." @default.
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- W2233590947 date "2015-12-31" @default.
- W2233590947 modified "2023-10-06" @default.
- W2233590947 title "Searching for X-ray sources in nearby late-type galaxies with low-star formation rates" @default.
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- W2233590947 doi "https://doi.org/10.1093/mnras/stv2888" @default.
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