2010
DOI: 10.7228/manchester/9780719082689.001.0001
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The Reality of Film

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Cited by 9 publications
(2 citation statements)
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“…It has also been suggested that the radio modulation is due to orbital changes in the lineof-sight free-free absorption of the stellar wind from the massive companion star (Brocksopp, Fender & Pooley 2002;Szostek & Zdziarski 2007). During the soft state, VLBI observations presented here have shown the jet flux at 4 cm is contained within ∼0.7 au which is approximately an order of magnitude smaller than in the hard state at the same wavelength (Rushton 2009). Therefore, the soft state quenching of the radio flux could be partly due to an increased absorption by the wind as the emission originates closer to the black hole and companion star.…”
Section: E V I D E N C E F O R a C O M Pac T J E T In A Soft Statementioning
confidence: 54%
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“…It has also been suggested that the radio modulation is due to orbital changes in the lineof-sight free-free absorption of the stellar wind from the massive companion star (Brocksopp, Fender & Pooley 2002;Szostek & Zdziarski 2007). During the soft state, VLBI observations presented here have shown the jet flux at 4 cm is contained within ∼0.7 au which is approximately an order of magnitude smaller than in the hard state at the same wavelength (Rushton 2009). Therefore, the soft state quenching of the radio flux could be partly due to an increased absorption by the wind as the emission originates closer to the black hole and companion star.…”
Section: E V I D E N C E F O R a C O M Pac T J E T In A Soft Statementioning
confidence: 54%
“…Targeted radio and X-ray observations of Cygnus X-1 were triggered after a series of Astronomer's Telegram 1 reports suggested a hardto-soft state transition was starting in late 2010 June (e.g. Negoro et al 2010;Rushton et al 2010;Sabatini et al 2010). Table 1 gives a summary of all long baseline radio observations and Fig.…”
Section: O B S E Rvat I O N S a N D R E S U Lt Smentioning
confidence: 99%