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The 1996 outburst of GRO J1655–40: the challenge of interpreting the multiwavelength spectra

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 300:1 (1998) 64-82

Authors:

RI Hynes, CA Haswell, CR Shrader, W Chen, Keith Horne, ET Harlaftis, K O'Brien, C Hellier, RP Fender
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Discovery of extended radio emission in the young cluster Wd1

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 299:4 (1998) l43-l47

Authors:

Clark, Fender, Waters, Dougherty, Koornneef, Steele, Van Blokland
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Radio observations of IRAS‐selected Southern hemisphere classical Be stars

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 299:4 (1998) 1119-1122

Authors:

Clark, Steele, Fender
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A radio survey of supersoft, persistent and transient X‐ray sources in the Magellanic Clouds

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 298:3 (1998) 692-696

Authors:

RP Fender, K Southwell, AK Tzioumis
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Infrared photometry and spectroscopy of the supersoft X-ray source RX J0019.8+2156 (= QR And)

Astronomy and Astrophysics 335:1 (1998)

Authors:

H Quaintrell, RP Fender

Abstract:

We present JHK photometry and spectroscopy of RX J0019.8+2156. The spectrum appears to be dominated by the accretion disc to at least 2.4 μm, over any other source of emission. We find Paschen, Brackett and He II lines strongly in emission, but no He I. There are satellite lines approximately 850km s-1 either side of the strongest, unblended hydrogen lines. These satellite lines may be the spectral signature of jets from the accretion disc.