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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| Publicado: |
1997
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v477_n1PARTII_pL45_Mirabel http://hdl.handle.net/20.500.12110/paper_0004637X_v477_n1PARTII_pL45_Mirabel |
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