High-Contrast NIR Polarization Imaging of MWC480

One of the key predictions of modeling from the IR excess of Herbig Ae stars is that for protoplanetary disks, where significant grain growth and settling has occurred, the dust disk has flattened to the point that it can be partially or largely shadowed by the innermost material at or near the dust...

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Veröffentlicht in:	arXiv.org 2012-05
Hauptverfasser:	Kusakabe, N, Grady, C A, Sitko, M L, Hashimoto, J, Kudo, T, Fukagawa, M, Muto, T, Wisniewski, J P, Min, M, Mayama, S, Werren, C, Day, A N, Beerman, L C, Lynch, D K, Russell, R W, Brafford, S M, Kuzuhara, M, Brandt, T D, Abe, L, Brandner, W, Carson, J, Egner, S, Feldt, M, Goto, M, Guyon, O, Hayano, Y, Hayashi, M, Hayashi, S S, Henning, T, Hodapp, K W, Ishii, M, Iye, M, Janson, M, Kandori, R, Knapp, G R, Matsuo, T, McElwain, M W, Miyama, S, J -I Morino, Moro-Martin, A, Nishimura, T, T -S Pyo, Suto, H, Suzuki, R, Takami, M, Takato, N, Terada, H, Thalmann, C, Tomono, D, Turner, E L, Watanabe, M, Yamada, T, Takami, H, Usuda, T, Tamura, M
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Dust Grain growth Imaging Physics - Solar and Stellar Astrophysics Planet formation Polarimetry Protoplanetary disks Protoplanets Scale height Spectral energy distribution Sublimation
Online-Zugang:	Volltext
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