Low-mass bare strange stars
Astrophysics
2007-05-23 v1
Abstract
Strange stars with low masses are suggested to exist in reality, the origin of which could be via accretion-induced collapse (AIC) of white dwarfs. Such a strange star is likely bare, and would thus spin very fast, even to a period of < 0.1 ms. Strange stars with low masses may differ from those with solar-masses in various astrophysical appearances. Observations to test this ``low-mass'' idea are proposed.
Keywords
Cite
@article{arxiv.astro-ph/0410652,
title = {Low-mass bare strange stars},
author = {R. X. Xu},
journal= {arXiv preprint arXiv:astro-ph/0410652},
year = {2007}
}
Comments
COSPAR-2004, E1.4, 6 pages