LI I 6708A BLEND IN THE SPECTRA OF STRONGLY MAGNETIC STAR HD166473

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...

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Bibliographic Details
Main Authors:	A. V. Shavrina, V. Khalack, Y. Glagolevskij, D. Lyashko, J. Landstreet, F. Leone, N. S. Polosukhina, M. Giarrusso
Format:	Article
Language:	English
Published:	Odessa I. I. Mechnykov National University 2013-11-01
Series:	Odessa Astronomical Publications
Online Access:	http://oap.onu.edu.ua/article/view/82294

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