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Massive Star and Star Cluster Formation

Jonathan C. Tan
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Abstract

I review the status of massive star formation theories: accretion from collapsing, massive, turbulent cores; competitive accretion; and stellar collisions. I conclude the observational and theoretical evidence favors the first of these models. I then discuss: the initial conditions of star cluster formation as traced by infrared dark clouds; the cluster formation timescale; and comparison of the initial cluster mass function in different galactic environments.

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Jonathan C. Tan. 2006-10-16. Massive Star and Star Cluster Formation. https://doi.org/10.1017/s1743921307001573

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