The surroundings of the superluminal source GRS 1915+105
We have carried out radio studies of the surroundings of the superluminal microquasar GRS 1915+105. Our main goal was to understand the possible relation of GRS 1915+105 with two infrared/radio sources that appear symmetrically located with respect to GRS 1915+105 and aligned with the position angle...
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todo:paper_00046361_v340_n2_pL47_Rodriguez2023-10-03T13:59:52Z The surroundings of the superluminal source GRS 1915+105 Rodríguez, L.F. Mirabel, I.F. ISM: HII regions ISM: Individual objects: IRAS 19124+1106, IRAS 19132+1035, SNR 45.7-0.4-ISM: supernova remnants X-rays:stars We have carried out radio studies of the surroundings of the superluminal microquasar GRS 1915+105. Our main goal was to understand the possible relation of GRS 1915+105 with two infrared/radio sources that appear symmetrically located with respect to GRS 1915+105 and aligned with the position angle of the relativistic ejecta. We have also studied a nearby supernova remnant to test if the event that created the remnant could have been the progenitor of this hard X-ray binary. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00046361_v340_n2_pL47_Rodriguez |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
ISM: HII regions ISM: Individual objects: IRAS 19124+1106, IRAS 19132+1035, SNR 45.7-0.4-ISM: supernova remnants X-rays:stars |
spellingShingle |
ISM: HII regions ISM: Individual objects: IRAS 19124+1106, IRAS 19132+1035, SNR 45.7-0.4-ISM: supernova remnants X-rays:stars Rodríguez, L.F. Mirabel, I.F. The surroundings of the superluminal source GRS 1915+105 |
topic_facet |
ISM: HII regions ISM: Individual objects: IRAS 19124+1106, IRAS 19132+1035, SNR 45.7-0.4-ISM: supernova remnants X-rays:stars |
description |
We have carried out radio studies of the surroundings of the superluminal microquasar GRS 1915+105. Our main goal was to understand the possible relation of GRS 1915+105 with two infrared/radio sources that appear symmetrically located with respect to GRS 1915+105 and aligned with the position angle of the relativistic ejecta. We have also studied a nearby supernova remnant to test if the event that created the remnant could have been the progenitor of this hard X-ray binary. |
format |
JOUR |
author |
Rodríguez, L.F. Mirabel, I.F. |
author_facet |
Rodríguez, L.F. Mirabel, I.F. |
author_sort |
Rodríguez, L.F. |
title |
The surroundings of the superluminal source GRS 1915+105 |
title_short |
The surroundings of the superluminal source GRS 1915+105 |
title_full |
The surroundings of the superluminal source GRS 1915+105 |
title_fullStr |
The surroundings of the superluminal source GRS 1915+105 |
title_full_unstemmed |
The surroundings of the superluminal source GRS 1915+105 |
title_sort |
surroundings of the superluminal source grs 1915+105 |
url |
http://hdl.handle.net/20.500.12110/paper_00046361_v340_n2_pL47_Rodriguez |
work_keys_str_mv |
AT rodriguezlf thesurroundingsofthesuperluminalsourcegrs1915105 AT mirabelif thesurroundingsofthesuperluminalsourcegrs1915105 AT rodriguezlf surroundingsofthesuperluminalsourcegrs1915105 AT mirabelif surroundingsofthesuperluminalsourcegrs1915105 |
_version_ |
1807316469006991360 |