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

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 1040 erg s−1; ref. 1) are thought to be powered by the accretion of gas onto black holes with masses of ~5–20 M☉, probably by means of an accretion disk. The X-ray and radio emission are coupled in such Galactic sources; t...

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Bibliographic Details
Main Authors: Middleton, Matthew J., Miller-Jones, James C. A., Markoff, Sera, Fender, Rob, Henze, Martin, Hurley-Walker, Natasha, Scaife, Anna M. M., Roberts, Timothy P., Walton, Dominic, Carpenter, John, Macquart, Jean-Pierre, Bower, Geoffrey C., Gurwell, Mark, Pietsch, Wolfgang, Haberl, Frank, Harris, Jonathan, Daniel, Michael, Miah, Junayd, Done, Chris, Morgan, John S., Dickinson, Hugh, Charles, Phil, Burwitz, Vadim, Della Valle, Massimo, Freyberg, Michael, Greiner, Jochen, Hernanz, Margarita, Hartmann, Dieter H., Hatzidimitriou, Despina, Riffeser, Arno, Sala, Gloria, Seitz, Stella, Reig, Pablo, Rau, Arne, Orio, Marina, Titterington, David, Grainge, Keith
Format: Journal Article
Published: Nature Publishing Group 2013
Subjects:
high-energy astrophysics
Online Access:http://hdl.handle.net/20.500.11937/28286

Internet

http://hdl.handle.net/20.500.11937/28286

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