EAS Publications Series
Volume 56, 2012The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?
|Page(s)||171 - 174|
|Section||Energizing the Disk-Halo: Star Formation, SNE, CRS and Feedback|
|Published online||17 September 2012|
Miguel A. de Avillez (ed)
EAS Publications Series, 56 (2012) 171–174
A High-Resolution Study of Two Galactic H I Halo Clouds in the Ophiuchus Superbubble
1 Joint Institute for VLBI in Europe, Postbus 2, 7990 AA, Dwingeloo, The Netherlands
2 National Radio Astronomy Observatory, PO Box 2, Green Bank, WV 24944, USA
3 National Radio Astronomy Observatory, PO Box 0, Socorro, NM 87801, USA
Two compact H I clouds which seem to belong to the Ophiuchus superbubble were studied at ∼30′′ resolution using the Very Large Array (VLA) in C and D configurations together with the Green Bank Telescope (GBT) providing the short-spacing flux. Here we present preliminary results of the data analysis.
© EAS, EDP Sciences, 2012