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NEAR-IR HIGH-RESOLUTION IMAGING POLARIMETRY OF THE SU Aur DISK: CLUES FOR TIDAL TAILS?

Jerome de Leon,Michihiro Takami,Jennifer L. Karr,Jun Hashimoto,Tomoyuki Kudo,Michael Sitko,Satoshi Mayama,Nobuyuki Kusakabe,Eiji Akiyama,Hauyu Baobab Liu,Tomonori Usuda,Lyu Abe,Wolfgang Brandner,Timothy D. Brandt,Joseph Carson,Thayne Currie,Sebastian E. Egner,Markus Feldt,Katherine Follette,Carol A. Grady,Miwa Goto,Olivier Guyon,Yutaka Hayano,Masahiko Hayashi,Saeko Hayashi,Thomas Henning,Klaus W. Hodapp,Miki Ishii,Masanori Iye,Markus Janson,Ryo Kandori,Gillian R. Knapp,Masayuki Kuzuhara,Jungmi Kwon,Taro Matsuo,Michael W. McElwain,Shoken Miyama,Jun-Ichi Morino,Amaya Moro-Martin,Tetsuo Nishimura,Tae-Soo Pyo,Eugene Serabyn,Takuya Suenaga,Hiroshi Suto,Ryuji Suzuki,Yasuhiro Takahashi,Naruhisa Takato,Hiroshi Terada,Christian Thalmann,Daigo Tomono,Edwin L. Turner,Makoto Watanabe,John P. Wisniewski,Toru Yamada,Hideki Takami,Motohide Tamura

The Astrophysical Journal（2015）

Cited 19|Views64
Key words
polarization,protoplanetary disks,stars: individual (SU Aur),stars: pre-main sequence
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