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Star Formation in the Spiral Galaxy M33

Published online by Cambridge University Press:  04 August 2017

F. Viallefond*
Affiliation:
Meudon Observatory, France

Extract

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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
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