Volume 367, Number 2, February IV 2001
|Page(s)||613 - 616|
|Published online||15 February 2001|
An attempt to identify the extended synchrotron structure associated with the micro-quasar GRS 1915+105
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, firstname.lastname@example.org
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.