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Low-column density HVC and IVC gas in the halo of the Milky Way

Published online by Cambridge University Press:  17 September 2012

N. Ben Bekhti ,
P. Richter ,
B. Winkel ,
F. Kenn ,
T. Westmeier  and
M. Murphy
N. Ben Bekhti
Affiliation:
Argelander-Institut für Astronomie, University of Bonn, Germany
P. Richter
Affiliation:
Institut für Physik und Astronomie, University of Potsdam, Germany
B. Winkel
Affiliation:
Argelander-Institut für Astronomie, University of Bonn, Germany
F. Kenn
Affiliation:
Argelander-Institut für Astronomie, University of Bonn, Germany
T. Westmeier
Affiliation:
Australia Telescope National Facility, CSIRO, Australia
M. Murphy
Affiliation:
Centre for Astrophysics & Supercomputing, Swinburne University of Technology, Australia
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Abstract

We analyse the distribution and physical properties of low-column density gas in the halo of the Milky Way with optical and UV absorption spectroscopy and with 21-cm observations.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 56: The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall? , 2012 , pp. 313 - 317
Copyright
© EAS, EDP Sciences, 2012

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References

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