Magnetic Massive Stars
2007 ◽
Vol 3
(S250)
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pp. 577-586
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Keyword(s):
The Past
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AbstractMagnetic fields are unexpected in massive stars, due to the absence of a sub-surface convective dynamo. However, advances in instrumentation over the past three decades have led to their detection in a small but growing subset of these stars. Moreover, complementary theoretical developments have highlighted their potentially significant influence over the structure, evolution and circumstellar environments of massive stars. Here, we summarize a special session convened prior to the main conference, focused on presenting recent developments in the study of massive-star magnetic fields.
2010 ◽
Vol 6
(S270)
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pp. 57-64
Keyword(s):
2020 ◽
Vol 493
(1)
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pp. 518-535
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Keyword(s):
2003 ◽
Vol 212
◽
pp. 38-46
Keyword(s):
2014 ◽
Vol 9
(S307)
◽
pp. 420-425
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Keyword(s):
2002 ◽
Vol 55
(4b)
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pp. 289-310
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1989 ◽
Vol 136
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pp. 171-177
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