Links

Results of spectropolarimetric observations of the supergiant ζ Ori are reported. The fast line profile variability (LPV) with a period of about 3 hours is found and a connection of LPV with a non-radial pulsation of the star is supposed. We did not find any evidence for a moderate stellar magnetic field as reported by Bouret et. al., 2008}.
Original languageEnglish
Title of host publicationMagnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev
PublisherСАО РАН
Pages355-360
StatePublished - 2011
Externally publishedYes

    Research areas

  • magnetic fields - stars

ID: 4545531