arXiv:astro-ph/9510073AbstractReferencesReviewsResources
Conversion of neutron stars to strange stars as an origin of gamma-ray bursts
Published 1995-10-14Version 1
This paper argues that conversion of neutron stars to strange stars as an origin of cosmological stars in the binaries with low-mass companions. Our model may provide an explanation why the binary millisecond pulsars seem to have same low magnetic fields.
Comments: 3 pages
Journal: Phys.Rev.Lett.77:1210-1213,1996
Categories: astro-ph
Tags: journal article
Related articles: Most relevant | Search more
arXiv:astro-ph/9812422 (Published 1998-12-22)
Gamma-Ray Bursts: the Four Crises
Quiescent times in gamma-ray bursts: II. Dormant periods in the central engine?
arXiv:astro-ph/9810220 (Published 1998-10-14)
On Source Density Evolution of Gamma-ray Bursts