On the Radiation Problem of High Mass Stars

Details On the Radiation Problem of High Mass Stars On the Radiation Problem of High Mass Stars

2008-07-18

arxiv.org/abs/0807.3035v5

Physics

General Physics

Published: Research in Astron. Astrophys. 2010 Vol. 10 No. 11, 1137-1150 (14 pages, 1 figure)

Scientific paper

We use the Azimuthally Symmetric Theory of Gravitation (set-forth in
arXiv:0912.2966 and further advanced in viXra:0911.0025) to argue that massive
stars must be able to form via the accretion disk without much problems.

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