Other
Scientific paper
Dec 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995aas...187.5503l&link_type=abstract
American Astronomical Society, 187th AAS Meeting, #55.03; Bulletin of the American Astronomical Society, Vol. 27, p.1366
Other
Scientific paper
In this talk the physical conditions within the recently discovered Galactic superluminal sources, GRS 1915+105 and GRO J1655+40, their interaction with their environment, and their possible formation will be examined, contrasting them with their extragalactic counterparts. In particular, the jet content, constraints on particle acceleration in the jets imposed using X-ray and radio observations, the gamma -ray flux from e(+) -e(-) jets expected at EGRET energies and the flux in infrared lines from an e-p jet will be discussed. The possibility that these sources may exhibit low frequency radio lobes extending up to several hundred parsecs in size, strong, soft X-ray absorption during the birth of the radio components, and emission line strengths anti- correlated with the X-ray flux will also be considered. Finally, the implications for other X-ray transients will be briefly discussed.
Blandford Roger
Levinson A. A.
No associations
LandOfFree
Physics of Galactic Superluminal Sources 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 Physics of Galactic Superluminal Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physics of Galactic Superluminal Sources will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1254516