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Magnetic fields in A stars besides Ap stars
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Observational Astronomy.
2014 (English)In: PUTTING A STARS INTO CONTEXT: EVOLUTION, ENVIRONMENT, AND RELATED STARS, 2014, 389-397 p.Conference paper, Published paper (Refereed)
Abstract [en]

I review ongoing efforts to understand the incidence of magnetism in intermediate-mass stars that are different from the magnetic Ap stars. This includes the search for magnetic fields in chemically peculiar stars of the Am and HgMn types as well as in normal A and late-B stars. I discuss different techniques for detecting weak stellar magnetic fields, and present a critical evaluation of recent magnetic detections in non-Ap stars. Special attention is given to the magnetic status of HgMn stars and to the discovery of weak polarization signatures in Sirius and Vega.

Place, publisher, year, edition, pages
2014. 389-397 p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-265980ISI: 000361017800056ISBN: 978-5-00086-273-5 (print)OAI: oai:DiVA.org:uu-265980DiVA: diva2:867074
Conference
International Conference on Putting A Stars into Context - Evolution, Environment, and Related Stars, JUN 03-07, 2013, Moscow, RUSSIA
Available from: 2015-11-04 Created: 2015-11-04 Last updated: 2015-11-04Bibliographically approved

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Kochukhov, Oleg

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