PREPRINT
E4C4927F-D316-4D7B-BEE5-FFDA7431272E

Open questions in massive star research

N. Langer

Submitted on 9 September 2022

Abstract

In discussing open question in the field of massive stars, I consider their evolution from birth to death. After touching upon massive star formation, which may be bi-modal and not lead to a zero-age main sequence at the highest masses, I consider the consequences of massive stars being close to their Eddington limit. Then, when discussing the effects of a binary companion, I highlight the importance of massive Algols and contact binaries for understanding the consequences of mass transfer, and the role of binaries in forming Wolf-Rayet stars. Finally, a discussion on pair instability supernovae and of superluminous supernovae is provided.

Preprint

Comment: to appear in Proceedings for IAU Symposium 361: Massive Stars Near and Far, held in Ballyconnell, Ireland, 9-13 May 2022, N. St-Louis, J. S. Vink & J. Mackey, eds

Subjects: Astrophysics - Solar and Stellar Astrophysics; Astrophysics - High Energy Astrophysical Phenomena

URL: https://arxiv.org/abs/2209.04165