Bright radio emission from an ultraluminous stellar-mass microquasar in M 31.

A subset of ultraluminous X-ray sources (those with luminosities of less than 10(40) erg s(-1); ref. 1) are thought to be powered by the accretion of gas onto black holes with masses of ∼5-20M cicled dot, probably by means of an accretion disk. The X-ray and radio emission are coupled in such Galact...

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Bibliographic Details
Main Authors:	Middleton, M, Miller-Jones, J, Markoff, S, Fender, R, Henze, M, Hurley-Walker, N, Scaife, A, Roberts, T, Walton, D, Carpenter, J, Macquart, J, Bower, G, Gurwell, M, Pietsch, W, Haberl, F, Harris, J, Daniel, M, Miah, J, Done, C, Morgan, J, Dickinson, H, Charles, P, Burwitz, V, Della Valle, M, Freyberg, M
Format:	Journal article
Language:	English
Published:	2013

Bright radio emission from an ultraluminous stellar-mass microquasar in M 31.

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