Title of article :
Of?p stars: a class of slowly rotating magnetic massive stars
Author/Authors :
Gregg A. Wade، نويسنده , , Jason H. Grunhut، نويسنده , , Wagner L. F. Marcolino، نويسنده , , Fabrice Martins، نويسنده , , Ian D. Howarth، نويسنده , , Yael Naze، نويسنده , , Nolan R. Walborn، نويسنده , , the MiMeS Collaboration، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2010
Pages :
2
From page :
220
To page :
221
Abstract :
Only 5 Of?p stars have been identified in the Galaxy. Of these, 3 have been studied in detail, and within the past 5 years magnetic fields have been detected in each of them. The observed magnetic and spectral characteristics are indicative of organised magnetic fields, likely of fossil origin, confining their supersonic stellar winds into dense, structured magnetospheres. The systematic detection of magnetic fields in these stars strongly suggests that the Of?p stars represent a general class of magnetic O-type stars.
Keywords :
stars: magnetic fields , stars: individual (HD 191612 , techniques: spectroscopic , HD 148937) , HD 108
Journal title :
Proceedings of the International Astronomical Union
Serial Year :
2010
Journal title :
Proceedings of the International Astronomical Union
Record number :
667848
Link To Document :
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