Hostname: page-component-8448b6f56d-42gr6 Total loading time: 0 Render date: 2024-04-18T00:25:25.312Z Has data issue: false hasContentIssue false
  • English
  • Français

The distribution of early-type stars in the Mon-CMa-Pup-Vel region of the Milky Way

Published online by Cambridge University Press:  01 August 2006

N. T. Kaltcheva
N. T. Kaltcheva*
Affiliation:
Department of Physics and Astronomy, University of Wisconsin Oshkosh, 800 Algoma Blvd., Oshkosh, WI 54901, USA email: kaltchev@uwosh.edu
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.

An overall uvby β photometric survey of the structure of the star-forming fields located toward the Monoceros-Canis Major-Puppis-Vela region of the Milky Way is presented.

Keywords

stars: distancesopen clusters and associations: generalGalaxy: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 431
Copyright
Copyright © International Astronomical Union 2007

References

Kaltcheva, N.T. & Hilditch, R. 2000, MNRAS 312, 753CrossRefGoogle Scholar
Kaltcheva, N.T. 2006, AN submittedGoogle Scholar