Long-term evolution of a magnetic massive merger product

ABSTRACT. About 10 per cent of stars more massive than ${\approx}1.5\, {\mathrm{M}}_{\odot }$ have strong, large-scale surface magnetic fields and are being di

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Bibliographic Details
Main Authors:	Schneider, Fabian (Author) , Ohlmann, Sebastian T. (Author) , Podsiadlowski, Philipp (Author) , Röpke, Friedrich (Author) , Balbus, Steven A. (Author) , Pakmor, Rüdiger (Author)
Format:	Article (Journal)
Language:	English
Published:	May 15, 2020
In:	Monthly notices of the Royal Astronomical Society Year: 2020, Volume: 495, Issue: 3, Pages: 2796-2812
ISSN:	1365-2966
DOI:	10.1093/mnras/staa1326
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa1326 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/495/3/2796/5837578
Author Notes:	F.R.N. Schneider, S.T. Ohlmann, Ph. Podsiadlowski, F.K. Röpke, S.A. Balbus and R. Pakmor

Description
Summary:	ABSTRACT. About 10 per cent of stars more massive than ${\approx}1.5\, {\mathrm{M}}_{\odot }$ have strong, large-scale surface magnetic fields and are being di
Item Description:	Gesehen am 10.08.2020
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/staa1326