Study of magnetic fields of different luminosity hot stars

Details Study of magnetic fields of different luminosity hot stars Study of magnetic fields of different luminosity hot stars

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mast.conf..247b&link_type=abstract

Magnetic stars, Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, Au

Astronomy and Astrophysics

Astrophysics

Magnetic Fields, Pulsations

Scientific paper

. Circular spectropolarimetric observations of four different luminosity hot stars were obtained in an attempt to detect magnetic fields via longitudinal Zeeman effect in the spectral line HeI 6678.149 Å: γ Pegasi (Sp B2 IV), γ Orionis (Sp B2 III), ω Orionis (Sp B3 IIIe), ζ Persei (Sp B1 Ib). No statistically significant values of the mean magnetic field were detected. The pulsation period of γ Pegasi was refined as P = 0d.151750393 ± 6.4 × 10-8

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