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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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Bibliographische Detailangaben
Hauptverfasser: Schneider, Fabian (VerfasserIn) , Ohlmann, Sebastian T. (VerfasserIn) , Podsiadlowski, Philipp (VerfasserIn) , Röpke, Friedrich (VerfasserIn) , Balbus, Steven A. (VerfasserIn) , Pakmor, Rüdiger (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: May 15, 2020
In: Monthly notices of the Royal Astronomical Society
Year: 2020, Jahrgang: 495, Heft: 3, Pages: 2796-2812
ISSN:1365-2966
DOI:10.1093/mnras/staa1326
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa1326
Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/495/3/2796/5837578
Volltext
Verfasserangaben:F.R.N. Schneider, S.T. Ohlmann, Ph. Podsiadlowski, F.K. Röpke, S.A. Balbus and R. Pakmor

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