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Magnetic fields in O-type stars measured with FORS 1 at the VLT
Stockholms universitet, Naturvetenskapliga fakulteten, Institutionen för astronomi. (Institute for Solar Physics)
Vise andre og tillknytning
2009 (engelsk)Inngår i: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, 2009, Vol. 259, s. 381-382Konferansepaper, Publicerat paper (Fagfellevurdert)
Abstract [en]

The presence of magnetic fields in O-type stars has been suspected for a long time. The discovery of such fields would explain a wide range of well documented enigmatic phenomena in massive stars, in particular cyclical wind variability, Hα emission variations, chemical peculiarity, narrow X-ray emission lines and non-thermal radio/X-ray emission. Here we present the results of our studies of magnetic fields in O-type stars, carried out over the last years.

sted, utgiver, år, opplag, sider
2009. Vol. 259, s. 381-382
Serie
Proc. IAU ; 259
Emneord [en]
Stars: early-type, stars: magnetic fields, techniques: polarimetric, stars: HD 36879, HD 148937, HD 152408, HD 164794, HD 191612
Identifikatorer
URN: urn:nbn:se:su:diva-35882OAI: oai:DiVA.org:su-35882DiVA, id: diva2:288435
Tilgjengelig fra: 2010-01-21 Laget: 2010-01-20 Sist oppdatert: 2011-02-15bibliografisk kontrollert

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