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Large scale Structure of HI in other Galaxies

Published online by Cambridge University Press:  03 August 2017

Thijs Van Der Hulst  and
Jurjen Kamphuis
Thijs Van Der Hulst
Affiliation:
Kapteyn Astronomical Institute, Postbus 800, NL-9700 AV Groningen, The Netherlands
Jurjen Kamphuis
Affiliation:
Kapteyn Astronomical Institute, Postbus 800, NL-9700 AV Groningen, The Netherlands

Abstract

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In this paper we discuss the large-scale structures (> 500 pc) of the neutral atomic hydrogen in the disk of nearby galaxies, with an emphasis on finding evidence for neutral gas features in the disk - halo interface. Most nearby galaxies studied in detail appear to have hole and shell type structures in their HI disks and several show evidence for gas at peculiar velocities, probably examples of gas streaming out of the disk into the halo. Not all of the observed phenomena can be explained by stellar winds and supernova explosions and other explanations will briefly be discussed.

Information

Type
II. The Disk-Halo Interface in Other Galaxies
Information
Symposium - International Astronomical Union , Volume 144: The Interstellar Disk-Halo Connection in Galaxies , 1991 , pp. 201 - 212
Copyright
Copyright © Kluwer 1991 

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