Rotationally modulated variations and the mean longitudinal magnetic field of the Herbig Ae star HD 101412

HUBRIG, S.; MIKULÁEK, Z; GONZALEZ, J. F.; SCHÖLLER, M.; ILYIN, I.; CURÉ, M.; ZEJDA, M.; COWLEY, C. R.; ELKIN, V.; POGODIN, M. A.; YUDIN, R. V.

ASTRONOMY AND ASTROPHYSICS

EDP SCIENCES S A

Año: 2011 vol. 525 p. 4 - 9

0004-6361

Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, thesefields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lackof knowledge of their rotation periods. The sharp-lined young Herbig Ae star HD 101412 with a strong surface magnetic field hasbecome in the past few years one of the most well-studied targets among the Herbig Ae/Be stars.Aims. We present our multi-epoch polarimetric spectra of this star acquired with FORS 2 to search for a rotation period and constrainthe geometry of the magnetic field.Methods. We measured longitudinal magnetic fields for 13 different epochs distributed over 62 days. These new measurements andour previous measurements of the magnetic field in this star were combined with available photometric observations to determine therotation period.Results. We find the rotation period to be P = 42.076 ± 0.017 d. According to near-infrared imaging studies, the star is observednearly edge-on. The star exhibits a single-wave variation in the longitudinal magnetic field during the stellar rotation cycle. Theseobservations are usually considered as evidence of a dominant dipolar contribution to the magnetic field topology.