EDP Sciences
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201630149

Massive star formation by accretion. II. Rotation: how to circumvent the angular momentum barrier?

A&A, Forthcoming article
Received: 28 November 2016 / Accepted: 02 March 2017
DOI: https://doi.org/10.1051/0004-6361/201630149