Magnetospheric accretion in the intermediate-mass T Tauri star HQ Tauri

Context. Classical T Tauri stars are pre-main sequence stars surrounded by an accretion disk. They host a strong magnetic field, and both magnetospheric accretion and ejection processes develop as the young magnetic star interacts with its disk. Studying this interaction is a major goal toward under...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-10, Vol.642, p.A99
Hauptverfasser:	Pouilly, K., Bouvier, J., Alecian, E., Alencar, S. H. P., Cody, A.-M., Donati, J.-F., Grankin, K., Hussain, G. A. J., Rebull, L., Folsom, C. P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Astrophysics Binary stars Corotation Light curve Magnetic fields Magnetic stars Magnetospheres Photosphere Physics Polarimetry Pre-main sequence stars Radial velocity Stellar evolution Stellar magnetic fields Surface spots T Tauri stars
Online-Zugang:	Volltext
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