Fast-moving features in the debris disk around AU Microscopii.
Boccaletti A, Thalmann C, Lagrange AM, Janson M, Augereau JC, Schneider G, Milli J, Grady C, Debes J, Langlois M, Mouillet D, Henning T, Dominik C, Maire AL, Beuzit JL, Carson J, Dohlen K, Engler N, Feldt M, Fusco T, Ginski C, Girard JH, Hines D, Kasper M, Mawet D, Ménard F, Meyer MR, Moutou C, Olofsson J, Rodigas T, Sauvage JF, Schlieder J, Schmid HM, Turatto M, Udry S, Vakili F, Vigan A, Wahhaj Z, Wisniewski J.
Boccaletti A, et al.
Nature. 2015 Oct 8;526(7572):230-2. doi: 10.1038/nature15705.
Nature. 2015.
PMID: 26450055
This was proved to be true for the beta Pictoris system, in which the known planet generates an observable warp in the disk. The nearby, young, unusually active late-type star AU Microscopii hosts a well-studied edge-on debris disk; earlier observations in th …
This was proved to be true for the beta Pictoris system, in which the known planet generates an observable warp in the disk. The near …