Evolution of Young Stellar Objects

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 01 Jan 2012Publisher:Springer Berlin Heidelberg

Authors: Norbert S. Schulz;

doi: 10.1007/978-3-642-23926-7_6

Evolution of Young Stellar Objects

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Abstract

This chapter decribes the evolution of stellar objects after the PMF phase when a young stellar object forms via accretion from its circumstellar cloud. It is difficult, if not impossible, to draw a line between the process of protostellar formation and the evolution of a protostar toward a mature star on the main sequence. The dense central object that forms during the collapse of a cloud core is not yet a star, but it is also not a molecular core anymore.

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