Magneto-hydrodynamical origin of eclipsing time variations in post-common-envelope binaries for solar mass secondaries

Navarrete, Felipe H.; Schleicher, Dominik R. G.; Käpylä, Petri J.; Schober, Jennifer; Völschow, Marcel; Mennickent, Ronald E.

doi:10.1093/mnras/stab836

Publisher DOI:	10.1093/mnras/stab836 10.1093/mnras/stz3065 10.48550/arXiv.1906.06787
Title:	Magneto-hydrodynamical origin of eclipsing time variations in post-common-envelope binaries for solar mass secondaries
Language:	English
Authors:	Navarrete, Felipe H. Schleicher, Dominik R. G. Käpylä, Petri J. Schober, Jennifer Völschow, Marcel Mennickent, Ronald E.
Keywords:	Binaries: eclipsing; Dynamo; Methods: numerical; MHD; Stars: rotation; astro-ph.SR; astro-ph.SR
Issue Date:	27-Apr-2021
Publisher:	Oxford Univ. Press
Journal or Series Name:	Monthly notices of the Royal Astronomical Society
Volume:	491
Issue:	1
Startpage:	1043
Endpage:	1056
URI:	https://hdl.handle.net/20.500.12738/17560
ISSN:	1365-2966
Review status:	This version was peer reviewed (peer review)
Institute:	Department Informations- und Elektrotechnik Fakultät Technik und Informatik
Type:	Article
Additional note:	Preprint: https://doi.org/10.48550/arXiv.1906.06787. Verlagsversion, Version 1: https://doi.org/10.1093/mnras/stz3065. Verlagsversion, Version 2: https://doi.org/10.1093/mnras/stab836.
Appears in Collections:	Publications without full text