Hostname: page-component-5c6d5d7d68-wpx84 Total loading time: 0 Render date: 2024-08-08T07:31:33.461Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Luminosity Function of Open Clusters Containing Wolf-Rayet Stars

Published online by Cambridge University Press:  03 August 2017

A.G. Admiranto  and
B. Hidayat
A.G. Admiranto
Affiliation:
1National Institute of Aeronautics and Space (LAPAN), Bandung, West-Java, Indonesia
B. Hidayat
Affiliation:
2Observatorium Bosscha, Institute of Technology Bandung, Lembang, West-Java, Indonesia

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.

It is generally accepted that mass loss and overshooting are the two main processes that play important roles in the formation of Wolf-Rayet stars (Chiosi & Maeder, 1986). Such mechanisms modify the interior of a star. We cannot, however, disregard the possibility that there are external factors, which can influence the formation and evolution of Wolf-Rayet stars.

Type
Session VIII. Inventory and Distribution
Information
Symposium - International Astronomical Union , Volume 143: Wolf–Rayet Stars and Interrelations with other Massive Stars in Galaxies , 1991 , pp. 643
Copyright
Copyright © Kluwer 1991 

References

Lundström, I., Stenholm, B. 1984, Astron. Astrophys. Suppl. 58, 163.Google Scholar
Burki, G. 1977, Astron. Astrophys. 57, 135.Google Scholar
Chiosi, C., Maeder, A. 1986, Ann. Rev. Astron. Astrophys. 24, 329.Google Scholar