Search Publications

Gamma rays from accreting matter onto collapsed objects
DOI: 10.1016/0273-1177(84)90113-3 Bibcode: 1984AdSpR...3j.335K

Giovannelli, F.; Karakula, S.; Tkaczyk, W.

In the spherical accretion onto massive objects, the matter may be heated up to temperatures as high as 1012 °K. In such a hot plasma, the thermal bremsstrahlung (e-e and e-p) and π° decay from inelastic collisions of protons are the main γ-ray sources. We determined the γ -ray production spectra from the π° decay and from bremsstrahlun…

1984 Advances in Space Research
COS-B 6
Studies of high-latitude gamma rays
DOI: 10.1016/0273-1177(84)90068-1 Bibcode: 1984AdSpR...3j..87S

Strong, A. W.

COS-B gamma-ray data (70-5000 MeV) in the latitude range 10°< b <90° are compared with the expected emission from cosmic-ray interactions with interstellar gas. An additional component is found to be necessary to explain the latitude dependence of the emission. Two possible origins for this component are discussed: a gamma-ray halo around th…

1984 Advances in Space Research
COS-B 6
Rapid short-term pulse-period variations in Vela X-1 (4U 0900-40)
DOI: 10.1016/0273-1177(84)90057-7 Bibcode: 1984AdSpR...3j..39V

van der Klis, M.; Bonnet-Bidaud, J. M.

Results are presented of an analysis of 83 days of 2-12 keV X-ray observations of Vela X-1 (4U 0900-40) obtained during three separate pointings with the ESA COS-B satellite. The pulsation period is shown to undergo very rapid intrinsic changes, at a rate of up to P˙/P ~ 10-1 yr-1 during intervals of a few days. The lower val…

1984 Advances in Space Research
COS-B 2
The radial distribution of gamma rays and cosmic rays in the outer Galaxy
DOI: 10.1016/0273-1177(84)90067-X Bibcode: 1984AdSpR...3j..83H

Hermsen, W.; Bloemen, J. B. G. M.; Blitz, L.

The radial distribution of the high-energy (70 MeV-5 GeV) gamma-ray emissivity in the outer Milky Way is derived. The kinematics of HI are used to construct column-density maps in three galacto-centric distance ranges in the outer Galaxy. These maps are used in combination with COS-B gamma-ray data to determine gamma-ray emissivities in these dist…

1984 Advances in Space Research
COS-B 1
The galactic distribution of cosmic-ray particles
DOI: 10.1016/0273-1177(84)90337-5 Bibcode: 1984AdSpR...4b.393H

Hermsen, W.; Bloemen, J. B. G. M.

COS-B gamma-ray observations are compared with large-scale HI and CO surveys in different regions of the sky to derive information on the cosmic-ray density distribution throughout the Galaxy and/or a calibration of the ratio between H2 column density and integrated CO line intensity [N(H2)/Wco]. In the region of t…

1984 Advances in Space Research
COS-B 0
Background-sensitive event selection in the search for gamma-ray sources
DOI: 10.1016/0273-1177(84)90070-X Bibcode: 1984AdSpR...3j..95O

Özel, M. E.; Mayer-Haßelwander, H. A.

Poor angular resolution of present day gamma ray telescopes (1° at 100 MEV) together with the complicated gamma ray sky structures at compareable angular extents and poor statistics available necessitate the selection of those gammas which will increase the observable signal from a suspected source. A method for such a selection using the pre-know…

1984 Advances in Space Research
COS-B 0