Formation of long-period post-common-envelope binaries I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence stars

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Belloni, Diogo, Zorotovic, Monica, Schreiber, Matthias R., Parsons, Steven G., Moe, Maxwell, Garbutt, James A.
Format:	Preprint
Published:	2024
Subjects:	Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Internet

https://arxiv.org/abs/2401.07692