Results of Magnetic Field Measurements Performed with the 6-m Telescope. IV. Observations in 2010
arXiv:1803.09957 · doi:10.1134/S1990341317040046
Abstract
We present the results of measurements of magnetic fields, radial velocities and rotation velocities for 92 objects, mainly main-sequence chemically peculiar stars. Observations were performed at the 6-m BTA telescope using Main Stellar Spectrograph with a Zeeman analyzer. In 2010, twelve new magnetic stars were discovered: HD\,17330, HD\,29762, HD\,49884, HD\,54824, HD\,89069, HD\,96003, HD\,113894, HD\,118054, HD\,135679, HD\,138633, HD\,138777, BD\,+53.1183. The presence of a field is suspected in HD\,16705, HD\,35379 and HD\,35881. Observations of standard stars without a magnetic field confirm the absence of systematic errors which can introduce distortions into the measurements of longitudinal field. The paper gives comments on the results of investigation of each star.
References in corpus (7)
- Weak magnetic fields in Ap/Bp stars: Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy
- The MiMeS survey of magnetism in massive stars: Magnetic analysis of the O-type stars
- The extraordinary complex magnetic field of the helium-strong star HD 37776
- The FORS1 catalogue of stellar magnetic field measurements
- Evolution of magnetic fields in stars across the upper main sequence: I. Catalogue of magnetic field measurements with FORS1 at the VLT
- HD 178892 - a cool Ap star with extremely strong magnetic field
- Comprehensive study of the magnetic stars HD 5797 and HD 40711 with large chromium and iron overabundances
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- A new sample of super-slowly rotating Ap (ssrAp) stars from the Zwicky Transient Facility survey
- Super-slowly rotating Ap (ssrAp) stars: New spectroscopic observations
- Magnetic field measurements of sharp-lined Ap stars
- Discovery of eight 'Main-sequence Radio Pulse emitters' using the GMRT: clues to the onset of coherent radio emission in hot magnetic stars