Titlebook: High Energy Phenomena Around Collapsed Stars; F. Pacini Book 1987 D Reidel Publishing Company, Dordrecht, Holland 1987 Bulge.Galaxy.LOPES.

依法逮捕

Radio Supernovae, data set, we investigate the class properties of the RSN and derive descriptive parameters for the gross features of their radio “l(fā)ight curves.” These are then applied to the several models available for the phenomenon to investigate their relative merits and their relations to the various types an

Mortal

Picks-Disease

Plerions in Theory and in Practice, end products of stellar evolution. Here we review the main features of the currently accepted plerion model, including some recent variants. The model allows a quantitative study of some individual objects, and of the statistical properties of the class.

廢墟

The Binary Origin of Pulsar Velocities,ulsars belong to a class characterized by low velocities and low magnetic fields. These were significantly spun-up by accretion and released from the binary through a non-explosive disruption of the companion. The rest belong to the high velocity, high magnetic field class. Using relations between t

毗鄰

Black Holes in our Galaxy,scussed, as well as the possibility of electromagnetic extraction of spin energy from Kerr holes. The results are relevant both to binary X-ray sources, and also to “l(fā)one” black holes which may abound in the Galactic Disc and Halo.

音樂會(huì)

,“Gamma — Ray Sources in our Galaxy”,the hope of opening a new window of observational astronomy which was to shed new “l(fā)ight” on a variety of energetic astrophisical processes in compact objects as well as in the interstellar medium (ISM).

我悲傷

Cosmic Gamma Ray Bursts,ed. The observational evidence for a neutron star origin is discussed. The characteristics of some of the time histories and energy spectra argue strongly in favor of such an origin, but firm evidence, say in the form of an identifiable counterpart, is still lacking.

Flavouring

Galactic Cosmic Rays: Propagation and Origin, spallation reactions in the interstellar medium, are well accounted for by simple models where cosmic rays escape from the galaxy and/or from their source in an energy dependent way; this may be due to the scattering of cosmic rays by resonant irregularities resulting from the general interstellar

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睨視

Recent Developments on the Crab Nebula,lium abundance, no clear anomalies have been firmly established. Because of this and because of the uncertainty in the distance, the nature of SN 1054 remains in doubt. There are important asymmetries in the kinematics and composition of the shell and in the energy input into the Nebula.