| Issue |
EAS Publications Series
Volume 56, 2012
The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?
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|---|---|---|
| Page(s) | 313 - 317 | |
| Section | The Active Disk-Halo Connection: Infall vs. Outflows | |
| DOI | https://doi.org/10.1051/eas/1256051 | |
| Published online | 17 September 2012 | |
The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?
Miguel A. de Avillez (ed)
EAS Publications Series, 56 (2012) 313–317
Miguel A. de Avillez (ed)
EAS Publications Series, 56 (2012) 313–317
Low-column density HVC and IVC gas in the halo of the Milky Way
1 Argelander-Institut für Astronomie, University of Bonn, Germany
2 Institut für Physik und Astronomie, University of Potsdam, Germany
3 Australia Telescope National Facility, CSIRO, Australia
4 Centre for Astrophysics & Supercomputing, Swinburne University of Technology, Australia
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.
© EAS, EDP Sciences, 2012