LI I 6708A BLEND IN THE SPECTRA OF STRONGLY MAGNETIC STAR HD166473
The analysis of Li I 6708 Ǻ blend in the spectra of HD166473 was performed for 6 rotational phases distributed over the whole rotational period (P~9.5 years). The magnetic field model has been constructed based on the polarimetric measurements from Mathys et al. (2007). For each observed phase the...
Main Authors: | , , , , , , , |
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Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2013-11-01
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Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/82294 |