Hot Subdwarfs: Magnetic, Oscillatory and Other Physical Properties
作者： R. Oreiro , F. Pérez Hernández , M. Manteiga , A. Ulla , J. M. González Pérez
DOI: 10.1007/978-94-017-0799-2_36
关键词:
摘要: Hot subdwarf stars (hot sds) are blue subluminous objects. Only a few determinations available to date regarding the study of such aspects as rotation, microturbulent velocities or magnetic nature these Over 26 sdBs known be multiperiodic rapid oscillators. This project presents preliminary results new observations and models sample pulsating non-pulsating hot sds, including considerations on mass loss eventual properties.
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