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A weak compact jet ...
A weak compact jet in a soft state of Cygnus X-1
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- Rushton, Anthony, 1983 (author)
- Chalmers tekniska högskola,Chalmers University of Technology
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- Miller-Jones, J. C. A. (author)
- Curtin University
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- Campana, R. (author)
- Istituto nazionale di astrofisica (INAF)
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- Evangelista, Y. (author)
- Istituto nazionale di astrofisica (INAF)
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- Paragi, Z. (author)
- Joint Institute for VLBI in Europe (JIVE),Magyar Tudomanyos Akademia,Hungarian Academy of Sciences
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- Maccarone, T. J. (author)
- University of Southampton
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- Pooley, G. G. (author)
- University Of Cambridge
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- Tudose, V. (author)
- Netherlands Institute for Radio Astronomy (ASTRON),Academia Romana
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- Fender, R. P. (author)
- University of Southampton
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- Spencer, R. E. (author)
- University of Manchester
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- Dhawan, V. (author)
- National Radio Astronomy Observatory Socorro
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(creator_code:org_t)
- 2011-11-22
- 2012
- English.
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In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 419:4, s. 3194-3199
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http://dx.doi.org/10...
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https://academic.oup...
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Abstract
Subject headings
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- We present evidence for the presence of a weak compact jet during a soft X-ray state of Cygnus X-1. Very-high-resolution radio observations were taken with the VLBA, EVN and MERLIN during a hard-to-soft spectral state change, showing the hard state jet to be suppressed by a factor of about 35 in radio flux and unresolved to direct imaging observations (i.e. ?1 mas at 4 cm). High time-resolution X-ray observations with the RXTE-PCA were also taken during the radio monitoring period, showing the source to make the transition from the hard state to a softer state (via an intermediate state), although the source may never have reached the canonical soft state. Using astrometric very long baseline interferometry (VLBI) analysis and removing proper motion, parallax and orbital motion signatures, the residual positions show a scatter of similar to 0.2 mas (at 4 cm) and similar to 3 mas (at 13 cm) along the position angle of the known jet axis; these residuals suggest that there is a weak unresolved outflow, with varying size or opacity, during intermediate and soft X-ray states. Furthermore, no evidence was found for extended knots or shocks forming within the jet during the state transition, suggesting that the change in outflow rate may not be sufficiently high to produce superluminal knots.
Subject headings
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Keyword
- X-rays: binaries
- grs 1915+105
- variability
- gx 339-4
- radio-emission
- ISM: jets and outflows
- relativistic jet
- vlbi observations
- efficient
- black-holes
- x-ray binaries
- orbital modulation
- stars: individual: Cygnus X-1
Publication and Content Type
- art (subject category)
- ref (subject category)
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- By the author/editor
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Rushton, Anthony ...
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Miller-Jones, J. ...
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Campana, R.
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Evangelista, Y.
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Paragi, Z.
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Maccarone, T. J.
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show more...
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Pooley, G. G.
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Tudose, V.
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Fender, R. P.
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Spencer, R. E.
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Dhawan, V.
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show less...
- About the subject
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- NATURAL SCIENCES
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NATURAL SCIENCES
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and Physical Science ...
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and Astronomy Astrop ...
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Monthly Notices ...
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Chalmers University of Technology