On the Radiation Problem of High Mass Stars
arXiv:0807.3035
Abstract
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.
Published: Research in Astron. Astrophys. 2010 Vol. 10 No. 11, 1137-1150 (14 pages, 1 figure)