期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 411, 期 1, 页码 L41-L45出版社
WILEY-BLACKWELL
DOI: 10.1111/j.1745-3933.2010.00988.x
关键词
hydrodynamics; ISM: bubbles; planetary nebulae: general; planetary nebulae: individual: NGC 7293
资金
- Science and Technology Facilities Council [ST/I001557/1, ST/H008802/1, ST/F002092/1] Funding Source: researchfish
- STFC [ST/I001557/1, ST/F002092/1, ST/H008802/1] Funding Source: UKRI
A new mechanism for the formation of cometary tails behind dense clouds or globules is discussed. Numerical hydrodynamical models show that when a dense shell of swept-up matter overruns a cloud, material in the shell is focused behind the cloud to form a tail. This mode of tail formation is completely distinct from other methods, which involve either the removal of material from the cloud or shadowing from a strong, nearby source of ionization. This mechanism is relevant to the cometary tails seen in planetary nebulae and to the interaction of superbubble shells with dense clouds.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据