D 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

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
Name: Předpovědi rychlosti ztráty hmoty horkých hvězd
Investor: Czech Science Foundation, Mass-loss rate predictions for hot stars
MEB0810095, research and development project
Name: Nové trendy ve výzkumu geometricky proměnných hvězd
Investor: Ministry of Education, Youth and Sports of the CR, Programme KONTAKT - mobilities (MEB)
MUNI/A/0968/2009, interní kód MU
Name: Fyzika hvězd a hvězdných soustav (Acronym: FYHA)
Investor: Masaryk University, Category A