Stellar Collisions and Pulsar Planets
| dc.creator | Hansen, Brad M. S. | |
| dc.date | 2000-08-16 | |
| dc.date.accessioned | 2026-07-07T01:54:56Z | |
| dc.date.available | 2026-07-07T01:54:56Z | |
| dc.description | I describe models for the formation of planetary systems surrounding the remnants of stellar mergers and collisions. I focus primarily on models for the viscous evolution of disks suitable for the formation of the planets surrounding the pulsar B1257+12. I show that the adaptation of models for traditional protoplanetary disks which invoke quiescent or `dead' zones are quite successful in producing disks appropriate for the formation of the pulsar planets. I also briefly describe some even more exotic possibilities that may arise from compact object mergers. | |
| dc.description | Tex, 17 pages, including 6 postscript figures To appear in: Stellar Collisions, Mergers and their Consequences, ASP Conference Series, Ed. M. Shara | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0008226 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0008226 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1483 | |
| dc.subject | Astrophysics | |
| dc.title | Stellar Collisions and Pulsar Planets | |
| dc.type | text |