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• W3100157918 endingPage "A55" @default.
• W3100157918 startingPage "A55" @default.
• W3100157918 abstract "Context. Based mostly on stellar models that do not include rotation, CO white dwarfs that accrete helium at rates of about ~10-8M⊙/ yr have been put forward as candidate progenitors for a number of transient astrophysical phenomena, including Type Ia supernovae and the peculiar and fainter Type Iax supernovae." @default.
• W3100157918 created "2020-11-23" @default.
• W3100157918 creator A5017927399 @default.
• W3100157918 creator A5021040079 @default.
• W3100157918 creator A5039268655 @default.
• W3100157918 date "2017-06-01" @default.
• W3100157918 modified "2023-09-27" @default.
• W3100157918 title "Helium ignition in rotating magnetized CO white dwarfs leading to fast and faint rather than classical Type Ia supernovae" @default.
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• W3100157918 doi "https://doi.org/10.1051/0004-6361/201630121" @default.
• W3100157918 hasPublicationYear "2017" @default.
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