Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-24T01:44:32.648Z Has data issue: false hasContentIssue false
  • English
  • Français

Star Formation in the Spiral Galaxy M33

Published online by Cambridge University Press:  04 August 2017

F. Viallefond
F. Viallefond*
Affiliation:
Meudon Observatory, France

Extract

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 spiral galaxy M33 has been observed at several frequencies from the ultraviolet to the radio regions. The observations at 2030 A have been presented by Milliard (1984); the radio data obtained with the WSRT and the VLA are presented and analyzed in a series of papers (Viallefond and Goss 1986, and references therein).

Type
II. Large Scale Processes of Star Formation
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 624 - 625
Copyright
Copyright © Reidel 1987 

References

Milliard, B.: 1984, , University of Marseille.Google Scholar
Viallefond, F., and Goss, W.M.: 1986, Astron. Astrophys. 154, 357.Google Scholar