Magnetometry of the classical T Tauri star GQ Lup: non-stationary dynamos and spin evolution of young Suns-Reference-Cited by-同舟云学术

Magnetometry of the classical T Tauri star GQ Lup: non-stationary dynamos and spin evolution of young Suns

Author:

Donati J.-F.¹,Gregory S. G.²,Alencar S. H. P.³,Hussain G.⁴,Bouvier J.⁵,Dougados C.⁵,Jardine M. M.⁶,Ménard F.⁵,Romanova M. M.⁷

Affiliation:

1. IRAP-UMR 5277; CNRS & Univ. de Toulouse; 14 Av. E. Belin; F-31400; Toulouse; France

2. California Institute of Technology; MC 249-17; Pasadena; CA; 91125; USA

3. Departamento de Fìsica-ICEx-UFMG; Av. Antônio Carlos; 6627; 30270-901; Belo Horizonte; MG; Brazil

4. ESO; Karl-Schwarzschild-Str. 2; D-85748; Garching; Germany

5. IPAG-UMR 5274; CNRS & Univ. J. Fourier; 414 rue de la Piscine; F-38041; Grenoble; France

6. School of Physics and Astronomy; University of St Andrews; St Andrews; KY16 9SS

7. Department of Astronomy; Cornell University; Ithaca; NY; 14853-6801; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference38 articles.

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