Detailed Information on Publication Record
2011
The Exceptional Herbig Ae star HD 101412
HUBRIG, Swetlana, Zdeněk MIKULÁŠEK, J. M. GONZÁLES, Marcus SCHÖLLER, I. ILYIN et. al.Basic information
Original name
The Exceptional Herbig Ae star HD 101412
Name in Czech
Výjimečná Herbigova Ae hvězda HD 101412
Authors
HUBRIG, Swetlana (276 Germany), Zdeněk MIKULÁŠEK (203 Czech Republic, guarantor, belonging to the institution), J. M. GONZÁLES (32 Argentina), Marcus SCHÖLLER (276 Germany), I. ILYIN (643 Russian Federation), M. CURÉ (32 Argentina), Miloslav ZEJDA (203 Czech Republic, belonging to the institution), Charles R. COWLEY (840 United States of America), V. G. ELKIN (643 Russian Federation), M. A. POGODIN (643 Russian Federation) and R. V. YUDIN (643 Russian Federation)
Edition
Moskva, Rusko, Magnetic Stars, p. 175-178, 4 pp. 2011
Publisher
EDP Sciences
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Russian Federation
Confidentiality degree
není předmětem státního či obchodního tajemství
Publication form
printed version "print"
RIV identification code
RIV/00216224:14310/11:00050442
Organization unit
Faculty of Science
ISBN
978-5-7422-3156-1
Keywords (in Czech)
hvězdy: atmosféry - hvězdy: individuální: HD 101412 - hvězdy: proměnné: obecně - hvězdy: rotace
Keywords in English
stars: magnetic field - stars: pre-main sequence - stars: atmospheres - stars: individual: HD 101412 - stars: variables: general - stars: rotation
Tags
International impact, Reviewed
Změněno: 28/1/2013 10:04, doc. RNDr. Miloslav Zejda, Ph.D.
Abstract
V originále
A few months ago we obtained multi-epoch polarimetric spectra of HD 101412 with the FORS2 to search for a rotation period and to constrain the geometry of the magnetic field. The search of the rotation period resulted in P = 42.076 +/- 0.017 d. Using stellar fundamental parameters and the longitudinal magnetic field phase curve, we discuss the magnetic field geometry. According to the near-infrared imaging studies, the star is observed nearly edge-on. The magnetic field geometry can likely be described by a centered dipole with a polar magnetic field strength B_{d} between 1.5 and 2 kG and an inclination beta of the magnetic axis to the rotation axis of 84 +/- 13.
Links
GA205/08/0003, research and development project |
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MEB0810095, research and development project |
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MUNI/A/0968/2009, interní kód MU |
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