Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-22T01:59:47.065Z Has data issue: false hasContentIssue false
  • English
  • Français

Chandra observations of massive star forming regions

Published online by Cambridge University Press:  08 November 2005

Ettore Flaccomio
Ettore Flaccomio
Affiliation:
INAF–Osservatorio Astronomico di Palermo, Piazza del Parlamento, 1, Palermo, Italy
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.

I review selected results obtained using Chandra X-ray observations of high mass star forming regions. Discussed topics include diffuse X-ray emission; the mechanism of X-ray emission in stars from the highest to the lowest masses; the role of imaging X-ray observations in the identification of star forming region members and the implications for star formation studies. Special attention will be given to results recently obtained for the Orion Nebula Cluster by the Chandra Orion Ultradeep Project (COUP).

Keywords

stars: activitystars: formationX-rays: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S227: Massive Star Birth: A Crossroads of Astrophysics , May 2005 , pp. 247 - 256
Copyright
© 2005 International Astronomical Union