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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
; | | Date: |
18 Aug 1997 | | Subject: | astro-ph | | Affiliation: | Univ. Sussex, UK), C.R. Shrader, W. Chen (NASA/GSFC), K. Horne, E.T. Harlaftis, K. O’Brien (Univ. St. Andrews, UK), C. Hellier (Univ. Keele, UK), J. Kemp (Univ. Columbia, NY | | 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. | | Source: | arXiv, astro-ph/9708158 | | Services: | Forum | Review | PDF | Favorites | |
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