HUBRIG, Swetlana, Marcus SCHÖLLER, I. ILYIN, Charles R. COWLEY, Zdeněk MIKULÁŠEK, Beate STELZER, M. A. POGODIN, Ruslan V. YUDIN and M. CURÉ. Characterising the magnetic fields of the Herbig Ae/Be stars HD 97048, HD 150193, HD 176386, and MWC 480. Astronomy and Astrophysics. Les Ulis Cedex, France: EDP Sciences, 2011, vol. 536, A45, p. 1-8. ISSN 0004-6361. Available from: https://dx.doi.org/10.1051/0004-6361/201117407.
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Basic information
Original name Characterising the magnetic fields of the Herbig Ae/Be stars HD 97048, HD 150193, HD 176386, and MWC 480
Name in Czech Charakteristiky magnetických polí Herbigových Ae/Be hvězd HD 97048, HD 150193, HD 176386 a MWC 480
Authors HUBRIG, Swetlana (276 Germany), Marcus SCHÖLLER (276 Germany), I. ILYIN (643 Russian Federation), Charles R. COWLEY (840 United States of America), Zdeněk MIKULÁŠEK (203 Czech Republic, guarantor, belonging to the institution), Beate STELZER (276 Germany), M. A. POGODIN (643 Russian Federation), Ruslan V. YUDIN (643 Russian Federation) and M. CURÉ (152 Chile).
Edition Astronomy and Astrophysics, Les Ulis Cedex, France, EDP Sciences, 2011, 0004-6361.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher France
Confidentiality degree is not subject to a state or trade secret
Impact factor Impact factor: 4.587
RIV identification code RIV/00216224:14310/11:00054479
Organization unit Faculty of Science
Doi http://dx.doi.org/10.1051/0004-6361/201117407
UT WoS 000298485100092
Keywords in English stars: pre-main sequence;stars: atmospheres; stars: magnetic field; stars: variables: general; stars: general
Tags AKR, rivok
Tags International impact, Reviewed
Changed by Changed by: Ing. Andrea Mikešková, učo 137293. Changed: 28/3/2012 11:09.
Abstract
Our search for periodicities resulted in P = 0.693 d for HD 97048, P = 1.317 d for HD 150193, and P = 0.899 d for HD 176386. The magnetic field geometry can likely be described by a centred dipole with a polar magnetic field strength Bd of several hundred Gauss. The longitudinal magnetic-field measurements of MWC 480 reveal the presence of a strong kG field, which was undetected in our previous low-resolution polarimetric observations with FORS 1.
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