VERTICAL STRUCTURE OF A SUPERNOVA-DRIVEN TURBULENT, MAGNETIZED INTERSTELLAR MEDIUM-Reference-Cited by-同舟云学术

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VERTICAL STRUCTURE OF A SUPERNOVA-DRIVEN TURBULENT, MAGNETIZED INTERSTELLAR MEDIUM

Published:2012-04-20 Issue:2 Volume:750 Page:104
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Hill Alex S.,Ryan Joung M.,Mac Low Mordecai-Mark,Benjamin Robert A.,Matthew Haffner L.,Klingenberg Christian,Waagan Knut

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/750/i=2/a=104/pdf

Reference77 articles.

1. Disc-halo interaction -- I. Three-dimensional evolution of the Galactic disc

2. Volume filling factors of the ISM phases in star forming galaxies

3. Global dynamical evolution of the ISM in star forming galaxies

4. Testing Global ISM Models: A Detailed Comparison of O vi Column Densities with FUSE and Copernicus Data

5. The photoelectric heating mechanism for very small graphitic grains and polycyclic aromatic hydrocarbons

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