Discovery of extended radio emission in the young cluster Wd1
(1998)
Observation of B+→ωK+ and Search for Related B Decays Modes
Physical Review Letters American Physical Society (APS) 81:2 (1998) 272-276
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.A limit on the mass of the ντ
Physics Letters B Elsevier 431:1-2 (1998) 209-218
A limit on the mass of the ν
Physics Letters B Elsevier BV 431:1-2 (1998) 209-218