The fragmentation of expanding shells: cloud formation rates and masses

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

The gravitational instability of expanding shells is discussed. Linear and nonlinear terms are included in an analytical solution in the static and homogeneous medium. We discuss the interaction of modes and give the time needed for fragmentation. Masses of individual fragments are also estimated and their formation rates and the initial mass function are derived. Results of simulations are compared to observation.
3 pages, 4 figures, to appear in IAU Symposium Series, Vol. 207

Keywords

Astrophysics

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/2885

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0106156
 http://arxiv.org/abs/astro-ph/0106156

Collections

arXiv