Volume 578, June 2015
|Number of page(s)||4|
|Published online||16 June 2015|
Real-time evolution of a large-scale relativistic jet
Dept. de Física, EPS de Jaén, Universidad de Jaén,
Campus Las Lagunillas s/n, A3-402,
2 Dept. de Ingeniería Mecánica y Minera, EPS de Jaén, Universidad de Jaén, Campus Las Lagunillas s/n, A3-402, 23071 Jaén, Spain
3 Instituto Argentino de Radioastronomía, C.C.5, 1894 Villa Elisa, Buenos Aires, Argentina
4 Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900, La Plata, Argentina
5 Grupo de Investigación FQM-322, Universidad de Jaén, Campus Las Lagunillas s/n, A3-065, 23071 Jaén, Spain
Received: 19 April 2015
Accepted: 21 May 2015
Context. Astrophysical jets are ubiquitous in the Universe on all scales, but their large-scale dynamics and evolution in time are hard to observe since they usually develop at a very slow pace.
Aims. We aim to obtain the first observational proof of the expected large-scale evolution and interaction with the environment in an astrophysical jet. Only jets from microquasars offer a chance to witness the real-time, full-jet evolution within a human lifetime, since they combine a “short”, few parsec length with relativistic velocities.
Methods. The methodology of this work is based on a systematic recalibraton of interferometric radio observations of microquasars available in public archives. In particular, radio observations of the microquasar GRS 1758−258 over less than two decades have provided the most striking results.
Results. Significant morphological variations in the extended jet structure of GRS 1758−258 are reported here that were previously missed. Its northern radio lobe underwent a major morphological variation that rendered the hotspot undetectable in 2001 and reappeared again in the following years. The reported changes confirm the Galactic nature of the source. We tentatively interpret them in terms of the growth of instabilities in the jet flow. There is also evidence of surrounding cocoon. These results can provide a testbed for models accounting for the evolution of jets and their interaction with the environment.
Key words: stars: jets / ISM: jets and outflows / X-rays: binaries / galaxies: jets / stars: individual: GRS 1758 / 258
© ESO, 2015
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.