The superluminal source GRS 1915+105: A high-mass X-ray binary?
We obtained K-band (2.0-2.5 μm) infrared spectra of the visually obscured superluminal source GRS 1915+105 at three different epochs of 1995, at times when it was detected as a hard X-ray source. The three spectra exhibit H I Brγ (2.167 μm) and He I (2.058 μm) emission lines. The spectral morphology...
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todo:paper_0004637X_v477_n1PARTII_pL45_Mirabel2023-10-03T14:01:41Z The superluminal source GRS 1915+105: A high-mass X-ray binary? Mirabel, I.F. Bandyopadhyay, R. Charles, P.A. Shahbaz, T. Rodríguez, L.F. Infrared: stars Stars: emission-line, Be X-rays: stars We obtained K-band (2.0-2.5 μm) infrared spectra of the visually obscured superluminal source GRS 1915+105 at three different epochs of 1995, at times when it was detected as a hard X-ray source. The three spectra exhibit H I Brγ (2.167 μm) and He I (2.058 μm) emission lines. The spectral morphology, absolute magnitude, and time variability of the infrared counterpart are consistent with the class of high-mass X-ray binaries that contain late Oe and early Be stars as mass donors. In GRS 1915+105 we have not detected the Doppler-shifted emission lines observed in the classic stellar source of relativistic jets, SS 433. We discuss why it may be more difficult in GRS 1915+105 than in SS 433 to detect emission lines from the jets. © 1997. The American Astronomical Society. All rights reserved. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v477_n1PARTII_pL45_Mirabel |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
Infrared: stars Stars: emission-line, Be X-rays: stars |
spellingShingle |
Infrared: stars Stars: emission-line, Be X-rays: stars Mirabel, I.F. Bandyopadhyay, R. Charles, P.A. Shahbaz, T. Rodríguez, L.F. The superluminal source GRS 1915+105: A high-mass X-ray binary? |
topic_facet |
Infrared: stars Stars: emission-line, Be X-rays: stars |
description |
We obtained K-band (2.0-2.5 μm) infrared spectra of the visually obscured superluminal source GRS 1915+105 at three different epochs of 1995, at times when it was detected as a hard X-ray source. The three spectra exhibit H I Brγ (2.167 μm) and He I (2.058 μm) emission lines. The spectral morphology, absolute magnitude, and time variability of the infrared counterpart are consistent with the class of high-mass X-ray binaries that contain late Oe and early Be stars as mass donors. In GRS 1915+105 we have not detected the Doppler-shifted emission lines observed in the classic stellar source of relativistic jets, SS 433. We discuss why it may be more difficult in GRS 1915+105 than in SS 433 to detect emission lines from the jets. © 1997. The American Astronomical Society. All rights reserved. |
format |
JOUR |
author |
Mirabel, I.F. Bandyopadhyay, R. Charles, P.A. Shahbaz, T. Rodríguez, L.F. |
author_facet |
Mirabel, I.F. Bandyopadhyay, R. Charles, P.A. Shahbaz, T. Rodríguez, L.F. |
author_sort |
Mirabel, I.F. |
title |
The superluminal source GRS 1915+105: A high-mass X-ray binary? |
title_short |
The superluminal source GRS 1915+105: A high-mass X-ray binary? |
title_full |
The superluminal source GRS 1915+105: A high-mass X-ray binary? |
title_fullStr |
The superluminal source GRS 1915+105: A high-mass X-ray binary? |
title_full_unstemmed |
The superluminal source GRS 1915+105: A high-mass X-ray binary? |
title_sort |
superluminal source grs 1915+105: a high-mass x-ray binary? |
url |
http://hdl.handle.net/20.500.12110/paper_0004637X_v477_n1PARTII_pL45_Mirabel |
work_keys_str_mv |
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1782029108794884096 |