Clumpy Flows in Protoplanetary and Planetary Nebulae
天体物理学
2007-05-23 v1
摘要
Many astrophysical flows occur in inhomogeneous media. We briefly discuss some general properties of the adiabatic and radiative inhomogeneous systems and discuss the relevance of those properties to the planetary nebulae systems. We then focus on radiative hypersonic bullets and the applicability of this model to planetary and protoplanetary systems such as CRL 618, NGC 6543, Hen 3-1475.
引用
@article{arxiv.astro-ph/0310286,
title = {Clumpy Flows in Protoplanetary and Planetary Nebulae},
author = {A. Y. Poludnenko and A. Frank and S. Mitran},
journal= {arXiv preprint arXiv:astro-ph/0310286},
year = {2007}
}
备注
4 pages, 2 figures. To appear in "Asymmetric Planetary Nebulae III", eds. M. Meixner, J. Kastner, N. Soker and B. Balick, 2004, ASP Conference Series, for higher resolution version and animations see http://www.pas.rochester.edu/~wma