| Issue |
A&A
Volume 367, Number 2, February IV 2001
|
|
|---|---|---|
| Page(s) | 613 - 616 | |
| Section | The Sun | |
| DOI | https://doi.org/10.1051/0004-6361:20000454 | |
| Published online | 15 February 2001 | |
An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105
1
Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul.Orla 171, 30-244 Kraków, Poland
2
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53-201 Bonn 1, Germany
Corresponding author: M. Ostrowski, mio@oa.uj.edu.pl
Received:
18
October
2000
Accepted:
6
November
2000
The energy ejected from the galaxy micro-quasar GRS 1915+105 in the form of jets is expected to lead to formation of an extended double lobe/hot-spot structure with an energy content comparable to an average supernova remnant. We used the Effelsberg 100 m telescope at 10.45 GHz in attempt to identify such structures. For this distant galactic plane source, no definite identification was possible, due to high confusion by numerous background sources; however, a few suspect structures were identified.
Key words: ISM: jets and outflows / shock waves / acceleration of particles / radio continum: ISM
© ESO, 2001
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