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• W3123455436 abstract "In this paper we discuss the recently discovered radio transient in the nuclear region of M,82. It has been suggested that this source is an X-ray binary, which, given the radio flux density, would require an X-ray luminosity, $L_{rm X},sim6times10^{42}$,erg,s$^{-1}$ if it were a stellar mass black hole that followed established empirical relations for X-ray binaries. The source is not detected in the analysis of the X-ray archival data. Using a 99% confidence level upper limit we find that $L_{rm X} leq 1.8 times 10^{37}$,erg,s$^{-1}$ and $1.5 times 10^{37}$,erg,s$^{-1}$, using powerlaw and disk blackbody models respectively. The source is thus unlikely to be a traditional microquasar, but could be a system similar to SS,433, a Galactic microquasar with a high ratio of radio to X-ray luminosity." @default.
• W3123455436 created "2021-02-01" @default.
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• W3123455436 date "2011-06-21" @default.
• W3123455436 modified "2023-09-23" @default.
• W3123455436 title "The unusual radio transient in M82: an SS 433 analogue?" @default.
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• W3123455436 doi "https://doi.org/10.1111/j.1745-3933.2011.01078.x" @default.
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