Search Publications
Missions
Journals
Publication Years
Cos-B X-Ray Observations of CYGNUS-X-3 - an Indications for Apsidal Motion
van der Klis, M.; Bonnet-Bidaud, J. M.
Results are presented of three ∼40 d COS-B X-ray observations of Cyg X-3. The shape of the 4.8 h light curve showed variations on all observational time scales. An ∼20 d periodicity was found in the arrival time of the minimum of the light curve, interpreted as apsidal motion of an orbit with an eccentricity of ∼0.03.
Evidence in the COS-B data for time-variable gamma-ray sources in the galactic plane
Caraveo, P. A.; Strong, A. W.; Hermsen, W. +7 more
Gamma Rays from Specific Molecular Clouds
Wolfendale, A. W.; Li, Ti-Pei; Issa, M. R. +1 more
The characteristics of specific local molecular clouds which may be visible in gamma-rays are examined. Data from the SAS II and COS B satellites are used to derive observed gamma-ray fluxes and flux limits. Conversions are made to a standard energy threshold of 100 MeV, and averages are taken. Results show that on the average, not much enhancemen…
COS-B gamma-ray measurements, cosmic rays and the local interstellar medium
Caraveo, P. A.; Bignami, G. F.; Strong, A. W. +6 more
The results of COS-B gamma ray, cosmic ray, and the local interstellar medium measurements are summarized, with particular regard for H I emissions at galactic longitude 240 deg. Significant quantities of atomic hydrogen are calculated from the local gamma ray emissivity, and the gamma ray emissivity spectrum is deconvolved from equations of the e…
New large-scale properties of the galactic gamma radiation observed by COS-B in the context of the diffuse emission within the galactic disc
Caraveo, P. A.; Bignami, G. F.; Hermsen, W. +7 more
IUE Spectroscopy of Dwarf M Stars
Byrne, P. B.
Far-UV wind line profile changes in the O-type star HD 175754.
Stalio, R.; Carrasco, L.; Costero, R.
Resonance line profile changes in far-UV spectra of HD 175754, obtained with the IUE satellite are reported. These changes are interpreted in terms of variations in the dynamics and density-ionization structure of the star's wind.
Ultraviolet observations of Jupiter from Earth-orbiting satellites
Moore, V.
The International Ultraviolet Explorer (IUE) has provided both improved spectral resolution and some spatial resolution for UV observations of Jupiter. Previous satellite observations have produced albedo curves for Jupiter showing the influence of Rayleigh scattering, and of some absorber(s) shortward of 2500Å on the UV spectrum. Constraints on t…
A differential measurement of the Lyman alpha emission from the giant planets using IUE
Encrenaz, T.; Combes, M.; Fricke, K. H. +1 more
The intensity of the resonantly scattered Ly-α line of the gian planets depends on the scattering column length of atomic hydrogen above the methane layer and on the incident solar flux. We have obtained measurements of the Ly-α brightness of Jupiter and Saturn on December 19, 1979, with a time difference of 111 minutes, which is only slightly lon…
Erratum - IUE Observation of Strong Ultraviolet Absorption in the Spectrum of the c2 White Dwarf L145-141
Koester, D.; Vauclair, G.; Wiedemann, V.