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Spectral and QPO analysis of GX5-1 at very high intensity
Kendziorra, E.; Staubert, R.; Collmar, W.
From a short EXOSAT observation of the bright low mass X-ray binary GX 5-1 we have derived information about the spectral and the QPO behaviour of this source during a very high intensity state. GX 5-1 was found to be on the `horizontal branch' in the hardness ratio/intensity diagram. The X-ray luminosity (1-20 keV) varied from 3.8 *10<…
Energy distribution and variability of BL Lac objects: Recent observations and a theoretical scheme
Maraschi, L.
Spectral properties of X-ray selected and radio-selected BL Lacs are discussed. The results provide a direct indication that the X-ray emission is more isotropic than the radio emission. Recent results of multifrequency observations of the brightest X-ray selected BL Lac object, PKS 2155-304, are reviewed, showing how the fast X-ray variability is…
X-ray time variability and luminosity correlations in BL lacertae objects
Maccagni, D.; Giommi, P.; Garilli, B. +2 more
We present the preliminary results of a study of the soft X-ray properties of a sample of 34 BL Lacertae objects observed with the the EXOSAT Observatory. Strong correlations between the X-ray, optical and radio fluxes have been found in the subsample of X-ray selected objects. X-ray variability is common and has been significantly detected in 14 …
SS Cygni: The mass accretion rate behaviour in quiescence and in outburst
Gaudenzi, S.; Giovannelli, F.; Claudi, R. +1 more
From the HeII λ1640 emission line equivalent width values in all good available IUE low resolution spectra, we have deduced the correspondent mass accretion rate values Mdot for SS Cygni, using the optically thick boundary-layer model by Patterson and Raymond 1985. The Mdot behaviour can be distinguished as follows:
1) in the rising and decli…Accretion disc boundary layers with white dwarfs
van der Woerd, Hans
The boundary layer between the accretion disc and white dwarf in non-magnetic cataclysmic variables is the major source of X-rays from these systems. Two modes of X-ray emission exist; at low accretion rates a thermal instability develops in the accreting matter and a hard X-ray emitting corona is formed around the white dwarf; at high accretion r…
Infrared to UV energy distribution of the black hole candidate LMC X-3: Observation of the accretion disk
Maraschi, L.; Tanzi, E. G.; Chiappetti, L. +4 more
LMC X-3 is a binary X-ray source which most probably hosts a black hole. Here, the authors present a preliminary report on observations of the source in the IR, optical, and UV bands. The observations allow to evidentiate the presence of the accretion disk surrounding the black hole.
Simulataneous X-ray and optical observations of LMC X-2
Motch, C.; Beuermann, K.; Pakull, M. +3 more
The X-ray source LMC X-2 was observed with EXOSAT for -8hours on February 2nd, 1984 with simultaneous photometric and spectroscopic optical coverage. The source was seen at a luminosity of Lx ~ 1.5 1038erg.s-1 with a mean X-ray spectrum which can be described equally well by either a superposition of a thermal emis…
Two new results on PSR 0833-45: (1) optical data on its birthplace, and (2) possible polarization in its high energy gamma-ray emission
Bignami, G. F.
Two new and completely different results are presented, both related to the Vela pulsar PSR 0833-45. In Part I, recent ESO optical images of the pulsar and its starfield are compared to the discovery plates, and used to set stringent upper limits on its proper motion and thus on its birthplace. Consequences are briefly explored. Part 2 refers to a…