A Nebula in Your Computer: Simulating the Physics and Chemistry of an H II Region

被引：0
作者：
Bisbas, Thomas G. [1 ]
机构：
[1] UCL, Dept Phys & Astron, London WC1E 6BT, England
来源：
LABYRINTH OF STAR FORMATION | 2014年 / 36卷
关键词：
TRIGGERED STAR-FORMATION; PHOTOIONIZATION; HYDRODYNAMICS; CODE;
D O I：
10.1007/978-3-319-03041-8_38
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this contribution we discuss about numerical modeling of nebulae. In particular we emphasize on the dynamical evolution of an H II region and on the chemical structure of a Photodissociation region. We do this by using the Smoothed Particles Hydrodynamics code SEREN and the recently developed astrochemistry code 3D-PDR. We show an example application by simulating a cometary globule using these two codes.
引用
收藏
页码：205 / 208
页数：4
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