Contribution from Astrophysics in the Next Decade: JWST
and Concurrent Facilities, Astrophysics and Space Science
Proceedings, 2009, ed. H. A. Thronson, M. Stiavelli, and A. G. G. M. Tielens
For a PDF version of the article, click here.
astro-ph/1009.1416
Abstract. Extreme star formation includes star formation in starbursts and regions forming super star clusters. We survey the current problems in our understanding of the star formation process in starbursts and super star clusters - initial mass functions, cluster mass functions, star formation efficiencies, and radiative feedback into molecular clouds - that are critical to our understanding of the formation and survival of large star clusters, topics that will be the drivers of the observations of the next decade.
Table of Contents
EXTREME STAR FORMATION IN THE LOCAL UNIVERSE
WHAT CONSTITUTES EXTREME STAR FORMATION IN THE LOCAL
UNIVERSE?
EXTREME STAR-FORMING REGIONS OF THE LOCAL UNIVERSE
INITIAL MASS FUNCTIONS AND THE MOST MASSIVE STARS IN
SSCs
WHAT ARE THE INITIAL CLUSTER MASS FUNCTIONS FOR
SSCs?
WHAT ENVIRONMENTS LEAD TO EXTREME STAR FORMATION?
SUPER STAR CLUSTER MORTALITY
RADIATIVE FEEDBACK: EFFECTS ON MOLECULAR CLOUDS AND
CHEMISTRY
REFERENCES