Quenched millimetre emission from Cygnus X-1 in a soft X-ray state
arXiv:astro-ph/0405141 · doi:10.1111/j.1365-2966.2004.07992.x
Abstract
We present millimetre wavelength observations of the black hole candidate X-ray binary Cygnus X-1 which indicate a suppression, or quenching, of the emission as the source switches to a softer X-ray state. Combining the data with those for another black hole candidate, XTE J1118+480, we demonstrate that the millimetre emission shows the same coupling to X-rays as the radio emission, although with a much stronger sensitivity to spectral shape. We therefore confirm the association of the millimetre emission with the jets in low/hard state black hole candidate X-ray binaries.
arXiv commentAccepted for publication in MNRAS
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- On the Origin of Radio Emission in the X-ray States of XTE J1650-500 during the 2001-2002 Outburst
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