pith. sign in

arxiv: astro-ph/9510073 · v1 · submitted 1995-10-14 · 🌌 astro-ph

Conversion of neutron stars to strange stars as an origin of gamma-ray bursts

classification 🌌 astro-ph
keywords starsconversionneutronoriginstrangearguesbinariesbinary
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.