On the mechanism of low-mass compact object formation
| dc.creator | Popov, S. B. | |
| dc.date | 2004-03-31 | |
| dc.date.accessioned | 2026-07-07T02:12:47Z | |
| dc.date.available | 2026-07-07T02:12:47Z | |
| dc.description | We suggest that low-mass compact objects (hadron stars, quark stars) with $M<1 M_{\odot}$ can appear only due to fragmentation of rapidly rotating proto-neutron stars. Such low-mass stars receive large kicks due to an explosion of a lighter companion in a pair of fragments, or due to dynamical ejection of one of the lighter components in the case when three bodies are formed. As far as low-mass compact objects are expected to be slowly cooling in all popular models of thermal evolution possible candidates are expected to be found among hot high velocity sources. | |
| dc.description | 4 pages, no figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0403710 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0403710 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7573 | |
| dc.subject | Astrophysics | |
| dc.title | On the mechanism of low-mass compact object formation | |
| dc.type | text |