How was the Mushroom‐shaped GW 123.4−1.5 Formed in the Galactic Disk?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference20 articles.
1. A Search for Narrow Vertical Structures in the Canadian Galactic Plane Survey
2. Self-consistent determinations of the total amount of matter near the sun
3. Disc-halo interaction -- I. Three-dimensional evolution of the Galactic disc
4. Mushroom-shaped Structures as Tracers of Buoyant Flow in the Galactic Disk
5. The Galactic Worm GW 123.4−1.5: A Mushroom-shaped H [CLC][CSC]i[/CSC][/CLC] Cloud
Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Cosmic Rays and Non-thermal Emission Induced by Accretion of Cool Gas onto the Galactic Disk;The Astrophysical Journal;2017-10-26
2. Evolution of superbubbles in a self-gravitating disc;Monthly Notices of the Royal Astronomical Society;2012-08-29
3. The orientations of molecular clouds in the outer Galaxy: evidence for the scale of the turbulence driver?;Monthly Notices of the Royal Astronomical Society;2009-09-21
4. Formation of Galactic Center Magnetic Loops;Publications of the Astronomical Society of Japan;2009-06-25
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