An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105

Details An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105 An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105

2000-12-19

arxiv.org/abs/astro-ph/0012410v1

Astronomy and Astrophysics

Astrophysics

LaTeX uses a new 2001 A&A macro, 4 pages, 2 figures, A&A accepted

Scientific paper

10.1051/0004-6361:20000454

The energy ejected from the galaxy micro-quasar GRS1915+105 in the form of jets is expected to lead to formation of an extended double lobe/hot-spot structure with the energy content comparable to an average supernova remnant. We used the Effelsberg 100m telescope at 10.45 GHz in attempt to identify such structures. For this distant galactic plane source any definite identification was not possible due to high confusion by numerous background sources, however, a few suspect structures were pointed out.

Affiliated with

Also associated with

No associations

Rating

An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105 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 An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-255939