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- W2123171418 abstract "The Type Ib supernova 2010O was recently discovered in the interacting starburst galaxy Arp 299. We present an analysis of two archival Chandra X-ray observations of Arp 299 taken before the explosion and show that there is a transient X-ray source at a position consistent with the supernova. Due to the diffuse emission, the background is difficult to estimate. We estimate the flux of the transient from the difference of the two X-ray images and conclude that the transient can be described by a 0.225-keV blackbody with a luminosity of for a distance of 41 Mpc. These properties put the transient in between the Galactic black hole binary XTE J1550−564 and the ultraluminous X-ray binaries NGC 1313 X-1 and X-2. The high level of X-ray variability associated with the active starburst makes it impossible to rule out a chance alignment. If the source is associated with the supernova, it suggests SN 2010O is the explosion of the second star in a Wolf–Rayet X-ray binary, such as Cyg X-3, IC 10 X-1 and NGC 300 X-1." @default.
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- W2123171418 date "2010-04-21" @default.
- W2123171418 modified "2023-09-26" @default.
- W2123171418 title "The Type Ib supernova 2010O: an explosion in a Wolf-Rayet X-ray binary?" @default.
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- W2123171418 doi "https://doi.org/10.1111/j.1745-3933.2010.00861.x" @default.
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