Artículo
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?" (1997) Astrophysical Journal. 477(1 PART II):L45-L48
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Abstract:
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.
Registro:
| Documento: | Artículo |
| Título: | The superluminal source GRS 1915+105: A high-mass X-ray binary? |
| Autor: | Mirabel, I.F.; Bandyopadhyay, R.; Charles, P.A.; Shahbaz, T.; Rodríguez, L.F. |
| Filiación: | Service d'Astrophysique/CEA, DSM/DAPNIA, Centre d'Etudes de Saclay, F-91191 Gif-sur-Yvette, France Instituto de Astronomía y Física del Espacio, Argentina Department of Astrophysics, University of Oxford, Nuclear Physics Building, Keble Road, Oxford OX1 3RH, United Kingdom Instituto de Astronomía, UNAM, Apdo. Postal 70-264, 04510 México, D.F., Mexico |
| Palabras clave: | Infrared: stars; Stars: emission-line, Be; X-rays: stars |
| Año: | 1997 |
| Volumen: | 477 |
| Número: | 1 PART II |
| Página de inicio: | L45 |
| Página de fin: | L48 |
| Título revista: | Astrophysical Journal |
| Título revista abreviado: | Astrophys. J. |
| ISSN: | 0004637X |
| Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v477_n1PARTII_pL45_Mirabel |
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Citas:
---------- APA ----------
Mirabel, I.F., Bandyopadhyay, R., Charles, P.A., Shahbaz, T. & Rodríguez, L.F. (1997) . The superluminal source GRS 1915+105: A high-mass X-ray binary?. Astrophysical Journal, 477(1 PART II), L45-L48.Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v477_n1PARTII_pL45_Mirabel [ ]
---------- CHICAGO ----------
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?" . Astrophysical Journal 477, no. 1 PART II (1997) : L45-L48.Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v477_n1PARTII_pL45_Mirabel [ ]
---------- MLA ----------
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?" . Astrophysical Journal, vol. 477, no. 1 PART II, 1997, pp. L45-L48.Recuperado de https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v477_n1PARTII_pL45_Mirabel [ ]
---------- VANCOUVER ----------
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?. Astrophys. J. 1997;477(1 PART II):L45-L48.Available from: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v477_n1PARTII_pL45_Mirabel [ ]
