Baryons in the relativistic jets of the stellar-mass black-hole candidate 4U 1630-47

María Díaz Trigo (), James C. A. Miller-Jones, Simone Migliari, Jess W. Broderick and Tasso Tzioumis
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María Díaz Trigo: European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany
James C. A. Miller-Jones: International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, Western Australia 6845, Australia
Simone Migliari: Departament d’Astronomia i Meteorologia, Universitat de Barcelona, Martí I Franquès 1, 08028 Barcelona, Spain
Jess W. Broderick: School of Physics and Astronomy, University of Southampton
Tasso Tzioumis: Australia Telescope National Facility, CSIRO, PO Box 76, Epping, New South Wales 1710, Australia

Nature, 2013, vol. 504, issue 7479, 260-262

Abstract: Doppler-shifted X-ray emission lines from highly-ionized atoms, appearing together with radio emission from the relativistic jets of the black-hole candidate X-ray binary 4U 1630-47, indicate that the X-ray emission lines arise in a jet travelling at approximately two-thirds the speed of light and imply that the jet contains baryons.

Date: 2013
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DOI: 10.1038/nature12672

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