SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:research.chalmers.se:42b3168d-0df3-49c9-a5c7-c4e9c9bd41b5"
 

Search: onr:"swepub:oai:research.chalmers.se:42b3168d-0df3-49c9-a5c7-c4e9c9bd41b5" > A weak compact jet ...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

A weak compact jet in a soft state of Cygnus X-1

Rushton, Anthony, 1983 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Miller-Jones, J. C. A. (author)
Curtin University
Campana, R. (author)
Istituto nazionale di astrofisica (INAF)
show more...
Evangelista, Y. (author)
Istituto nazionale di astrofisica (INAF)
Paragi, Z. (author)
Joint Institute for VLBI in Europe (JIVE),Magyar Tudomanyos Akademia,Hungarian Academy of Sciences
Maccarone, T. J. (author)
University of Southampton
Pooley, G. G. (author)
University Of Cambridge
Tudose, V. (author)
Netherlands Institute for Radio Astronomy (ASTRON),Academia Romana
Fender, R. P. (author)
University of Southampton
Spencer, R. E. (author)
University of Manchester
Dhawan, V. (author)
National Radio Astronomy Observatory Socorro
show less...
 (creator_code:org_t)
2011-11-22
2012
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 419:4, s. 3194-3199
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • 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)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view