Circular Polarization Observations and Magnetic Fields of O Stars

dc.contributor.authorSudnik, N. P.
dc.contributor.authorKholtygin, Alexander F.
dc.date.accessioned2016-12-04T20:38:29Z
dc.date.available2016-12-04T20:38:29Z
dc.date.issued2012
dc.description.abstractThe results of a search for line profile variability (LPV) and polarimetric line profile variability (pLPV) in spectra of O stars are reported. The observations were made with the 1.8-m telescope of the Korean Bohyunsan Optical Astronomical Observatory (BOAO) and the 1-m and 6-m telescopes of the Special Astrophysical Observatory (SAO), Russia. Regular LPV in the spectra of all program stars are found. We analyze the connection between the presence of magnetic field and nitrogen abundance anomalies, and the influence of weak magnetic fields on pLPV. The statistical properties of mean magnetic fields and magnetic fluxes of OB stars are studied.ru_RU
dc.identifier.urihttp://elib.bspu.by/handle/doc/17340
dc.language.isoenru_RU
dc.relation.ispartofseriesAIP Conf. Proc.;v. 1429, p. 114 (2012)
dc.subjectБГПУru_RU
dc.subjectline profilesru_RU
dc.subjectpolarizationru_RU
dc.subjectstarsru_RU
dc.subjectoscillationsru_RU
dc.subjectearly-typeru_RU
dc.subjectmagnetic fieldsru_RU
dc.titleCircular Polarization Observations and Magnetic Fields of O Starsru_RU
dc.typeArticleru_RU

Files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
Sudnik_N.pdf
Size:
4.32 MB
Format:
Adobe Portable Document Format

License bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
license.txt
Size:
105 B
Format:
Item-specific license agreed upon to submission
Description: