Low-mass bare strange stars
| dc.creator | Xu, R. X. | |
| dc.date | 2004-10-27 | |
| dc.date.accessioned | 2026-07-07T02:15:31Z | |
| dc.date.available | 2026-07-07T02:15:31Z | |
| dc.description | 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. | |
| dc.description | COSPAR-2004, E1.4, 6 pages | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0410652 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0410652 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8434 | |
| dc.subject | Astrophysics | |
| dc.title | Low-mass bare strange stars | |
| dc.type | text |