Hostname: page-component-848d4c4894-8bljj Total loading time: 0 Render date: 2024-07-06T15:44:07.359Z Has data issue: false hasContentIssue false
  • English
  • Français

Sequential Star Formation inside the Young Stellar Associations of the Magellanic Clouds

Published online by Cambridge University Press:  04 August 2017

M. C. Lortet ,
G. Testor ,
V. Niemela  and
M. Heydari-Malayeri
M. C. Lortet
Affiliation:
Observatoire de Paris, Section de Meudon, D.A.F., 92195-Meudon Principal Cedex, France
G. Testor
Affiliation:
Observatoire de Paris, Section de Meudon, D.A.F., 92195-Meudon Principal Cedex, France
V. Niemela
Affiliation:
Instituto de Astronomia y Fisica del Espacio, C.C. 67, Suc. 28, 1428 Buenos Aires, Argentina
M. Heydari-Malayeri
Affiliation:
European Southern Observatory, Casilla 19001, Santiago 19, Chile

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.

While much work has been devoted to the history of star formation in the Magellanic Clouds at large spatial and time scales, little has been done on the details of sequential formation at the scale of a few 106 or 107 years and of less than 1000 pc.

Type
II. Large Scale Processes of Star Formation
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 551
Copyright
Copyright © Reidel 1987