CAOSP abstracts, Volume: 48, No.: 1, year: 2018

Abstract: In this review I will summarise what we know about magnetic fields in stars and what the origin of these magnetic fields may be. I will address the issue of whether the magnetic flux is conserved from pre-main sequence to the compact star phase (fossil field origin) or whether fields may be dynamo generated during some stages of stellar evolution or perhaps during stellar merging events.

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Last update: February 06, 2018