Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-25T16:14:38.821Z Has data issue: false hasContentIssue false
  • English
  • Français

Molecular material in the Bubble of the Galactic Center

Published online by Cambridge University Press:  09 February 2017

Miguel Angel Requena Torres  and
Alberto Noriega-Crespo
Miguel Angel Requena Torres
Affiliation:
Space Telescope Science Institute San Martin Drive, Baltimore, United States of America email: [email protected]
Alberto Noriega-Crespo
Affiliation:
Space Telescope Science Institute San Martin Drive, Baltimore, United States of America email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Galactic Center (GC) is one of the more extreme environments in the Galaxy. The so call Bubble of the GC presents structures that do not match with the general behavior of the inner Central Molecular Zone (CMZ). In this work we study the molecular emission related to the observable ionized gas emitted by this Bubble. We find dense pockets of gas and bubble like structures in the velocity domain.

Keywords

Galaxy: centermolecular dataISM: bubbles
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S322: The Multi-Messenger Astrophysics of the Galactic Centre , July 2016 , pp. 156 - 157
Copyright
Copyright © International Astronomical Union 2017 

References

Molinari, S., Bally, J., Noriega-Crespo, A., et al. 2011, ApJ, 735, 33 Google Scholar
Henshaw, J. D., Longmore, S. N., Kruijssen, J. M. D., et al. 2016, MNRAS, 457, 2675 Google Scholar
Kruijssen, , Dale, , & Longmore, 2015, MNRAS, 447, 1059 Google Scholar
Simpson, J. P., Rubin, R. H., Colgan, S. W. J., et al. 2004, ApJ, 611, 338 Google Scholar
Sofue, Y. 2003, PASJ, 55, 445 CrossRefGoogle Scholar