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Observations of Fast-Moving Features in the Debris Disk of AU Mic on a Three-Year Timescale: Confirmation and New Discoveries

A. Boccaletti,E. Sezestre,A-M Lagrange,P. Thebault,R. Gratton,M. Langlois,C. Thalmann,M. Janson,P. Delorme,J-C Augereau,G. Schneider,J. Milli,C. Grady,J. Debes,Q. Kral,J. Olofsson,J. Carson,A. L. Maire,T. Henning,J. Wisniewski,J. Schlieder,C. Dominik,S. Desidera,C. Ginski,D. Hines,F. Menard,D. Mouillet,N. Pawellek,A. Vigan,E. Lagadec,H. Avenhaus,J-L Beuzit,B. Biller,M. Bonavita,M. Bonnefoy,W. Brandner,F. Cantalloube,G. Chauvin,A. Cheetham,M. Cudel,C. Gry,S. Daemgen,M. Feldt,R. Galicher,J. Girard,J. Hagelberg,P. Janin-Potiron,M. Kasper,H. Le Coroller,D. Mesa,S. Peretti,C. Perrot,M. Samland,E. Sissa,F. Wildi,A. Zurlo,S. Rochat,E. Stadler,L. Gluck,A. Origne,M. Llored,P. Baudoz,G. Rousset,P. Martinez,F. Rigal

Astronomy and Astrophysics（2018）

引用 53|浏览61
关键词
stars: individual: AU Mic,circumstellar matter,planetary systems,planet-disk interactions,techniques: high angular resolution,techniques: image processing
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