منابع مشابه
Neutron Stars in Supernova Remnants
In the following, we shall briefly summarize some facts and ideas concerning the presence of neutron stars in Supernova remnants. While sources similar to the Crab Nebula require the presence of a central energetic object, shell-type remnants such as Cas A are compatible with the presence of neutron stars releasing a weak relativistic wind. Supernova remnants are usually classified into two ext...
متن کاملNeutron Stars in Supernova Remnants and Beyond
We discuss a concept of off-centred cavity supernova explosion as applied to neutron star/supernova remnant associations and show how this concept could be used to preclude the anti-humane decapitating the Duck (G 5.4−1.2 + G 5.27−0.9) and dismembering the Swan (Cygnus Loop), as well as to search for a stellar remnant associated with the supernova remnant RCW86.
متن کاملNeutron Stars, Pulsars and Supernova Remnants: concluding remarks
More than 30 years have elapsed since the discovery of pulsars (Hewish et al. 1968) and the realization that they are connected with rotating magnetized neutron stars (Gold 1968; Pacini 1967, 1968). It became soon clear that these objects are responsible for the production of the relativistic wind observed in some Supernovae remnants such as the Crab Nebula. For many years, the study of pulsars...
متن کاملGravitational radiation from highly magnetized nascent neutron stars in supernova remnants
We consider the spin evolution of highly magnetized neutron stars in a hypercritical inflow just after their birth in supernovae. Presence of a strong magnetic field could deform the star and if the symmetry axis of the field is misaligned with that of stellar rotation, the star will be an emitter of gravitational wave. Here we investigate the possibility of gravitational radiation from such a ...
متن کاملHigh-Energy Gamma Rays from Neutron Stars in Supernova Remnants: From EGRET to GLAST
At least three pulsars in supernova remnants were detected at E > 100 MeV by EGRET on the Compton Gamma Ray Observatory. Efforts to search for additional pulsars in the EGRET data have been unsuccessful due to limited statistics. An example is the recently-discovered radio pulsar J2229+6114, where efforts to search the EGRET data using several different methods failed to find significant eviden...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1987
ISSN: 0074-1809
DOI: 10.1017/s0074180900160541