Preprint
Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks
Abstract
We present radiation hydrodynamic simulations of collapsing protostellar
cores with initial masses of 30, 100, and 200 M$_{\odot}$. We follow their
Authors
Klassen M; Pudritz R; Kuiper R; Peters T; Banerjee R
Publication date
March 23, 2016
DOI
10.48550/arxiv.1603.07345
Preprint server
arXiv