Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-30T17:44:51.297Z Has data issue: false hasContentIssue false
  • English
  • Français

New insights into the nature of mid-infrared emission associated with massive star formation: disks and outflow

Published online by Cambridge University Press:  01 August 2006

James M. De Buizer
James M. De Buizer*
Affiliation:
Gemini Observatory, Casilla 603, La Serena, Chile 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.

Recent observations in the mid-infrared (5-25 μm) of massive young stellar sources have yielded a surprising result: many show evidence of mid-infrared emission from outflows and jets. These observations correlate well with other larger-scale outflow indicators and their geometries, such as what is seen in shock-excited H2 and CO emission. In some cases these mid-infrared observations identify the local maser emission as outflow or jet related.

Keywords

ISM: jets and outflowsinfrared: ISMcircumstellar matterstars: early-type
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 407
Copyright
Copyright © International Astronomical Union 2007

References

de Buizer, J. M. 2006a, ApJ 642, L57CrossRefGoogle Scholar
de Buizer, J. M. 2006b, ApJ submittedGoogle Scholar
de Buizer, J. M. & Minier, V. 2005, ApJ 628, L151CrossRefGoogle Scholar
Sridharan, T. K., Williams, S. J. & Fuller, G. A. 2005, ApJ 631, L73CrossRefGoogle Scholar