Clustered vs. Isolated Star Formation
| dc.creator | Mac Low, Mordecai-Mark | |
| dc.date | 2000-12-26 | |
| dc.date.accessioned | 2026-07-07T01:57:10Z | |
| dc.date.available | 2026-07-07T01:57:10Z | |
| dc.description | I argue that star formation is controlled by supersonic turbulence, drawing for support on a number of 3D hydrodynamical and MHD simulations as well as theoretical arguments. Clustered star formation appears to be a natural result of a lack of turbulent support, while isolated star formation is a signpost of global turbulent support. | |
| dc.description | 7 pages, 5 figures, for publication in ASP Conf. Ser., Modes of Star Formation and the Origin of Field Populations, eds. Grebel & Brandner | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0012499 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0012499 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/2281 | |
| dc.subject | Astrophysics | |
| dc.title | Clustered vs. Isolated Star Formation | |
| dc.type | text |