The magnetic field topology of the weak-lined T Tauri star V410 Tauri: New strategies for Zeeman-Doppler imaging
- Author
- CARROLL, T. A1 ; STRASSMEIER, K. G1 ; RICE, J. B2 ; KÜNSTLER, A1
[1] Leibniz-Institute for Astrophysics Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
[2] Department of Physics, Brandon University, Brandon, Manitoba R7A 6A9, Canada - Source
Astronomy and astrophysics (Berlin. Print). 2012, Vol 548 ; A95.1-A95.14 ; 2 ; ref : 3/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- - methods: data analysis line: profiles stars: activity stars: magnetic field techniques: spectroscopicstars: pre-main sequence
- Keyword (fr)
- Activité stellaire Analyse donnée Analyse image Champ axisymétrique Champ intense Champ magnétique Champ température Cisaillement Corrélation spatiale Décomposition valeur singulière Etoile magnétique Etoile pré séquence principale Etoile rotation Etoile type T Tauri Intensité Modélisation Méthode régularisation Profil raie Raie Stokes Rotation différentielle Structure magnétique Topologie Transfert radiatif
- Keyword (en)
- Stellar activity Data analysis Image analysis Axisymmetric field High field Magnetic fields Temperature distribution Shear Spatial correlation Singular value decomposition Magnetic stars Pre-main-sequence stars Rotating star T Tauri stars Intensity Modelling Regularization method Line shape Stokes lines Differential rotation Magnetic structure Topology Radiative transfer
- Keyword (es)
- Campo asimétrico Correlación espacial Estrella rotación Intensidad Método regularización
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 26785989
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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