Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-12-23
Rev.Mex.Astron.Astrof.Ser.Conf. 20 (2004) 203-203
Astronomy and Astrophysics
Astrophysics
To appear in RevMexAA(SC) Conference Series, Proc. of IAU Colloquium 194, Compact Binaries in the Galaxy and Beyond, La Paz, M
Scientific paper
Cygnus X-3, among the Galactic X-ray binaries, is one of the brightest radio sources. Radio image as well as spectral analysis shows the presence of outflow in the form of jets. The SED in the X-ray band shows a complicated structure and evolution. Here we review some recent results of the correlation of the long-term radio and X-ray emission, in the various states of the source, with emphasis on the low (hard) state. We compare the results with those of other common Galactic microquasars, and attempt to provide a consistent picture of the accretion-ejection mechanism in these types of binaries.
Choudhury Monojit
Rao Ravi A.
No associations
LandOfFree
The Radio : X-ray Correlation of Cygnus X-3 and other Galactic Microquasars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Radio : X-ray Correlation of Cygnus X-3 and other Galactic Microquasars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Radio : X-ray Correlation of Cygnus X-3 and other Galactic Microquasars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-322757