A Solution to the Radiation Pressure Problem in the Formation of Massive Stars View Full Text


Ontology type: schema:Chapter      Open Access: True


Chapter Info

DATE

2014-01-28

AUTHORS

Rolf Kuiper , Hubert Klahr , Henrik Beuther , Thomas Henning

ABSTRACT

We review our recent studies demonstrating that the radiation pressure problem in the formation of massive stars can be circumvented via an anisotropy of the thermal radiation field. Such an anisotropy naturally establishes with the formation of a circumstellar disk. The required angular momentum transport within the disk can be provided by developing gravitational torques. Radiative Rayleigh-Taylor instabilities in the cavity regions – as previously suggested in the literature – are not required and are shown to be unlikely in the context of massive star formation. More... »

PAGES

379-383

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-319-03041-8_74

DOI

http://dx.doi.org/10.1007/978-3-319-03041-8_74

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1018438571


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