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The two magnetic components in the Herbig Ae SB2 system HD104237. / Järvinen, S. P.; Carroll, T. A.; Hubrig, S.; Ilyin, I.; Schöller, M.; Drake, N. A.; Pogodin, M. A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 486, No. 4, 01.07.2019, p. 5499-5503.

Research output: Contribution to journal › Article › peer-review

Harvard

Järvinen, SP, Carroll, TA, Hubrig, S, Ilyin, I, Schöller, M, Drake, NA & Pogodin, MA 2019, 'The two magnetic components in the Herbig Ae SB2 system HD104237', Monthly Notices of the Royal Astronomical Society, vol. 486, no. 4, pp. 5499-5503. https://doi.org/10.1093/mnras/stz1212

APA

Järvinen, S. P., Carroll, T. A., Hubrig, S., Ilyin, I., Schöller, M., Drake, N. A., & Pogodin, M. A. (2019). The two magnetic components in the Herbig Ae SB2 system HD104237. Monthly Notices of the Royal Astronomical Society, 486(4), 5499-5503. https://doi.org/10.1093/mnras/stz1212

Vancouver

Järvinen SP, Carroll TA, Hubrig S, Ilyin I, Schöller M, Drake NA et al. The two magnetic components in the Herbig Ae SB2 system HD104237. Monthly Notices of the Royal Astronomical Society. 2019 Jul 1;486(4):5499-5503. https://doi.org/10.1093/mnras/stz1212

Author

Järvinen, S. P. ; Carroll, T. A. ; Hubrig, S. ; Ilyin, I. ; Schöller, M. ; Drake, N. A. ; Pogodin, M. A. / The two magnetic components in the Herbig Ae SB2 system HD104237. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 486, No. 4. pp. 5499-5503.

BibTeX

@article{d6813bdc1fa14a4db5c1f33a2fea0a85,
title = "The two magnetic components in the Herbig Ae SB2 system HD104237",
abstract = "We present longitudinal magnetic field measurements (Bz) for the Herbig Ae primary and the T Tauri secondary in the SB2 system HD104237. These measurements were carried out using high spectral resolution observations obtained with the High Accuracy Radial velocity Planet Searcher in polarimetric mode, installed at the ESO La Silla 3.6m telescope. In agreement with previous studies of Herbig Ae stars, the longitudinal magnetic field in the primary is rather weak, ranging from 47 to 72 G. The secondary component possesses a variable, much stronger magnetic field, up to 600 G, as expected for a magnetically active T Tauri star. We estimated the rotation period of the primary, Prot = 4.33717 ± 0.00316 d (=104 ± 0.08 h), from metal line equivalent width variations.",
keywords = "Stars: individual: HD104237, Stars: magnetic field, Stars: pre-main-sequence, Stars: variables: T Tauri, Herbig Ae/Be, FIELDS, stars: magnetic field, STAR, stars: individual: HD?104237, stars: pre-main-sequence, stars: variables: T Tauri, Herbig Ae/Be",
author = "J{\"a}rvinen, {S. P.} and Carroll, {T. A.} and S. Hubrig and I. Ilyin and M. Sch{\"o}ller and Drake, {N. A.} and Pogodin, {M. A.}",
year = "2019",
month = jul,
day = "1",
doi = "10.1093/mnras/stz1212",
language = "English",
volume = "486",
pages = "5499--5503",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Wiley-Blackwell",
number = "4",

}

RIS

TY - JOUR

T1 - The two magnetic components in the Herbig Ae SB2 system HD104237

AU - Järvinen, S. P.

AU - Carroll, T. A.

AU - Hubrig, S.

AU - Ilyin, I.

AU - Schöller, M.

AU - Drake, N. A.

AU - Pogodin, M. A.

PY - 2019/7/1

Y1 - 2019/7/1

N2 - We present longitudinal magnetic field measurements (Bz) for the Herbig Ae primary and the T Tauri secondary in the SB2 system HD104237. These measurements were carried out using high spectral resolution observations obtained with the High Accuracy Radial velocity Planet Searcher in polarimetric mode, installed at the ESO La Silla 3.6m telescope. In agreement with previous studies of Herbig Ae stars, the longitudinal magnetic field in the primary is rather weak, ranging from 47 to 72 G. The secondary component possesses a variable, much stronger magnetic field, up to 600 G, as expected for a magnetically active T Tauri star. We estimated the rotation period of the primary, Prot = 4.33717 ± 0.00316 d (=104 ± 0.08 h), from metal line equivalent width variations.

AB - We present longitudinal magnetic field measurements (Bz) for the Herbig Ae primary and the T Tauri secondary in the SB2 system HD104237. These measurements were carried out using high spectral resolution observations obtained with the High Accuracy Radial velocity Planet Searcher in polarimetric mode, installed at the ESO La Silla 3.6m telescope. In agreement with previous studies of Herbig Ae stars, the longitudinal magnetic field in the primary is rather weak, ranging from 47 to 72 G. The secondary component possesses a variable, much stronger magnetic field, up to 600 G, as expected for a magnetically active T Tauri star. We estimated the rotation period of the primary, Prot = 4.33717 ± 0.00316 d (=104 ± 0.08 h), from metal line equivalent width variations.

KW - Stars: individual: HD104237

KW - Stars: magnetic field

KW - Stars: pre-main-sequence

KW - Stars: variables: T Tauri, Herbig Ae/Be

KW - FIELDS

KW - stars: magnetic field

KW - STAR

KW - stars: individual: HD?104237

KW - stars: pre-main-sequence

KW - stars: variables: T Tauri, Herbig Ae/Be

UR - http://www.scopus.com/inward/record.url?scp=85067916253&partnerID=8YFLogxK

UR - http://www.mendeley.com/research/two-magnetic-components-herbig-ae-sb2-system-hd104237

U2 - 10.1093/mnras/stz1212

DO - 10.1093/mnras/stz1212

M3 - Article

AN - SCOPUS:85067916253

VL - 486

SP - 5499

EP - 5503

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -

ID: 49048475