Locating the Accretion Footprint on a Herbig Ae Star: MWC 480

Autor: Th. Henning, H. Meusinger, David K. Lynch, Bruce E. Woodgate, M. Endres, J. C. Bouret, B. Donehew, Robert Petre, Sean D. Brittain, M. Troutmann, Francois Menard, Jacqueline McCleary, Amanda N. Day, Glenn Schneider, Dean C. Hines, Carol A. Grady, Kenji Hamaguchi, John P. Wisniewski, R. J. Rudy, Ray W. Russell, S. Kim, B. Stecklum, Michael L. Sitko, Gerard M. Williger, M. Clampin, David J. Wilner, Karen A. Collins, A. Shenoy, M. Sahu, M. D. Silverstone

Publikováno v: The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2010, 719, pp.1565
The Astrophysical Journal, American Astronomical Society, 2012, 719, pp.1565-1581. ⟨10.1088/0004-637X/719/2/1565⟩

Accretion is a fundamental process which establishes the dynamics of the protoplanetary disk and the final properties of the forming star. In solar-type stars, the star-disk coupling is determined by the magnetic field structure, which is responsible

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a65f12ec1bd47a250e210b17d9781331
https://hal.archives-ouvertes.fr/hal-00631904