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http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p133.pdf.
http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p133.pdf.
1. Laboratory for the Stellar Magnetism Study of SAO of the RAS - Home
Observations of stellar magnetic fields is a powerful method to study of different non-stationary effects in our Galaxy and behavior of plasma under astrophysical conditions. ... Investigations of stellar magnetism by means of Zeeman measurements of polarized spectra of different stars are one of the most significant observational programme on the 6-m telescope BTA of our Observatory. ... Laboratory for the Stellar Magnetism Study . ... Laboratory for the Stellar Magnetism Study of SAO of the RAS . ...
2. http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p473.pdf
Magnetic Stars, 2011, pp. ... We discuss our most recent determination of the rotational period from longitudinal magnetic field measurements and H variability -- the latter obtained from over a decade's worth of professional and amateur spectroscopic observations. ... We concluded that the dipolar field of HD 57682 is characterized by a polar strength of 1.7 kG, and a magnetic axis aligned within 10 to 50 of the rotation axis, depending on the inclination of the rotation axis to our line of sight. ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p473.pdf -- 332.3 Кб -- 11.08.2011
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