Massive Star Formation

Details Massive Star Formation Massive Star Formation

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26...18r&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Hii Regions, Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

Over the last decades our knowledge on the formation of solar-type stars has increased significantly. Among the next frontiers in the field we have the understanding of stellar formation at the extremes, that is, how are objects much more massive (OB stars) and much less massive (brown dwarfs) than the Sun formed. I will focus on the formation of massive stars, discussing if it can be understood simply as a scaled-up version of the formation of solar type stars, or if phenomena of different nature are involved.

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