Real-time evolution of a large-scale relativistic jet
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 interactio...
Autores principales: | , , , , |
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Formato: | Articulo Contribucion a revista |
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2015
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/86696 |
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I19-R120-10915-86696 |
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institution |
Universidad Nacional de La Plata |
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I-19 |
repository_str |
R-120 |
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SEDICI (UNLP) |
language |
Inglés |
topic |
Ciencias Astronómicas Galaxies: jets ISM: jets and outflows Stars: individual: GRS 1758,258 Stars: jets X-rays: binaries |
spellingShingle |
Ciencias Astronómicas Galaxies: jets ISM: jets and outflows Stars: individual: GRS 1758,258 Stars: jets X-rays: binaries Martí, Josep Luque Escamilla, Pedro L. Romero, Gustavo Esteban Sánchez Sutil, Juan R. Muñoz Arjonilla, Álvaro J. Real-time evolution of a large-scale relativistic jet |
topic_facet |
Ciencias Astronómicas Galaxies: jets ISM: jets and outflows Stars: individual: GRS 1758,258 Stars: jets X-rays: binaries |
description |
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. |
format |
Articulo Contribucion a revista |
author |
Martí, Josep Luque Escamilla, Pedro L. Romero, Gustavo Esteban Sánchez Sutil, Juan R. Muñoz Arjonilla, Álvaro J. |
author_facet |
Martí, Josep Luque Escamilla, Pedro L. Romero, Gustavo Esteban Sánchez Sutil, Juan R. Muñoz Arjonilla, Álvaro J. |
author_sort |
Martí, Josep |
title |
Real-time evolution of a large-scale relativistic jet |
title_short |
Real-time evolution of a large-scale relativistic jet |
title_full |
Real-time evolution of a large-scale relativistic jet |
title_fullStr |
Real-time evolution of a large-scale relativistic jet |
title_full_unstemmed |
Real-time evolution of a large-scale relativistic jet |
title_sort |
real-time evolution of a large-scale relativistic jet |
publishDate |
2015 |
url |
http://sedici.unlp.edu.ar/handle/10915/86696 |
work_keys_str_mv |
AT martijosep realtimeevolutionofalargescalerelativisticjet AT luqueescamillapedrol realtimeevolutionofalargescalerelativisticjet AT romerogustavoesteban realtimeevolutionofalargescalerelativisticjet AT sanchezsutiljuanr realtimeevolutionofalargescalerelativisticjet AT munozarjonillaalvaroj realtimeevolutionofalargescalerelativisticjet |
bdutipo_str |
Repositorios |
_version_ |
1764820489212002306 |