Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-14T17:18:10.306Z Has data issue: false hasContentIssue false
  • English
  • Français

Warm molecular gas in the M17 SW nebula

Published online by Cambridge University Press:  21 October 2010

J. P. Pérez-Beaupuits ,
M. Spaans ,
M. Hogerheijde  and
R. Güsten
J. P. Pérez-Beaupuits
Affiliation:
Kapteyn Astronomical Institute, PO Box 800, 9700 AV, Groningen, The Netherlands
M. Spaans
Affiliation:
Kapteyn Astronomical Institute, PO Box 800, 9700 AV, Groningen, The Netherlands
M. Hogerheijde
Affiliation:
Leiden Observatory, Leiden University, PO Box 9513, 2300 RA, Leiden, The Netherlands
R. Güsten
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany email: jp@astro.rug.nl
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.

High resolution maps of the 12CO J = 6 → 5 line and the [C I]3P2 →3P1 (370 μm) fine-structure transition in the Galactic nebula M17 SW are presented. The maps were obtained using the dual color multiple pixel receiver CHAMP+ on the APEX† telescope.

Keywords

galactic: ISMgalactic: individual: M17 SWmolecules: 12COatoms: [C I]
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 401
Copyright
Copyright © International Astronomical Union 2010