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The 1996 Outburst of GRO J1655-40

R. I. Hynes·C. A. Haswell·R. P. Fender·C. R. Shrader·W. Chen·K. Horne·E. T. Harlaftis·K. O'Brien·C. Hellier·J. Kemp
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Abstract

During 1996 the soft-X-ray transient and superluminal jet source GRO J1655-40 was observed in outburst with a multiwavelength campaign including HST, RXTE, CGRO and ground based facilities. Here we focus on a key question raised by the observations: where and how does the outburst optical flux originate? Any model must not only fit the optical spectra, but must account for the observation that X-ray fluxes continued to rise slowly while the optical flux declined, contrary to predictions of standard models for the outburst of SXTs and dwarf novae.

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R. I. Hynes, C. A. Haswell, R. P. Fender, C. R. Shrader, W. Chen, K. Horne, E. T. Harlaftis, K. O'Brien, C. Hellier, J. Kemp. 1997-08-18. The 1996 Outburst of GRO J1655-40. https://arxiv.org/abs/astro-ph/9708158

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