Toward Understanding Massive Star Formation

Details Toward Understanding Massive Star Formation Toward Understanding Massive Star Formation

2007-07-09

arxiv.org/abs/0707.1279v1

Ann.Rev.Astron.Astrophys.45:481-563,2007

Astronomy and Astrophysics

Astrophysics

139 pages, 18 figures, 5 tables, glossary

Scientific paper

10.1146/annurev.astro.44.051905.

Although fundamental for astrophysics, the processes that produce massive stars are not well understood. Large distances, high extinction, and short timescales of critical evolutionary phases make observations of these processes challenging. Lacking good observational guidance, theoretical models have remained controversial. This review offers a basic description of the collapse of a massive molecular core and a critical discussion of the three competing concepts of massive star formation: - monolithic collapse in isolated cores - competitive accretion in a protocluster environment - stellar collisions and mergers in very dense systems We also review the observed outflows, multiplicity, and clustering properties of massive stars, the upper initial mass function and the upper mass limit. We conclude that high-mass star formation is not merely a scaled-up version of low-mass star formation with higher accretion rates, but partly a mechanism of its own, primarily owing to the role of stellar mass and radiation pressure in controlling the dynamics.

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