Gamma-ray bursts from fast, Galactic neutron stars [electronic resource]
What makes a Galacic model of gamma-ray bursts (GBs) feasible is the observation of a new population of objects, fast neutron stars, that are isotropic with respect to the Galaxy following a finite period, {approximately}30My, after their formation. Our Galactic model for the isotropic component of...
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Online Access |
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| Format: | Government Document Electronic eBook |
| Language: | English |
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Washington, D.C. : Oak Ridge, Tenn. :
United States. Dept. of Energy ; distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy,
1995.
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Internet
Online AccessOnline
| Call Number: |
E 1.99:CONF-9504198--1
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| E 1.99:CONF-9504198--1 | Available |