Preprint
Massive star formation via high accretion rates and early disk-driven outflows
Abstract
We present an investigation of massive star formation that results from the
gravitational collapse of massive, magnetized molecular cloud cores. We
Authors
Banerjee R; Pudritz RE
Publication date
December 22, 2006
DOI
10.48550/arxiv.astro-ph/0612674
Preprint server
arXiv