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
Infrared photometry and spectroscopy of the supersoft X-ray source RX J0019.8+2156 (= QR And)
Astronomy and Astrophysics 335:1 (1998)
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.Deep multicolour imaging of the field towards the quasar pair PC1643+463 A&B
YOUNG UNIVERSE: GALAXY FORMATION AND EVOLUTION AT INTERMEDIATE AND HIGH REDSHIFT 146 (1998) 492-495
The variable radio emission from GRS 1915 + 105
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 292:4 (1997) 925-933