Winds of magnetic B stars

Details Winds of magnetic B stars Winds of magnetic B stars

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221...95b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 95-100

Astronomy and Astrophysics

Astronomy

11

B Stars, Magnetic Stars, Stellar Magnetospheres, Stellar Physics, Stellar Winds, Ultraviolet Astronomy, Ultraviolet Spectra, Balmer Series, H Alpha Line, Spectral Signatures, Stellar Magnetic Fields, Stellar Models

Scientific paper

The magnetic Bp stars, i.e., the helium-strong and helim-weak/silicon-strong stars, have well ordered, global magnetic fields and are hot enough to have weak, radiatively driven stellar winds. They are the only stars where we can study magnetic winds for which the approximate magnetic field structure is known. Magnetic winds are interesting in their own right. In addition, they provide an opportunity to look for unique signatures that can be used to identify magnetic winds in stars where the fields are too weak or complex to be observed directly.

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