@article{oai:ir.soken.ac.jp:00003309,
 author = {眞山, 聡 and MAYAMA, Satoshi and TAMURA, Motohide and HAYASHI, Masahiko and HAYASHI, Saeko S and ITOH, Yoichi and FUKAGAWA, Misato and SUTO, Hiroshi and ISHII, Miki and MURAKAWA, Koji and OASA, Yumiko and YAMASHITA, Takuya and MORINO, Junichi and OYA, Shin and NAOI, Takahiro and PYO, Tae-Soo and NISHIKAWA, Takayuki and KUDO, Tomoyuki and USUDA, Tomonori and ANDO, Hiroyasu and MIYAMA, Shoken M and KAIFU, Norio},
 issue = {2},
 journal = {Publications of the Astronomical Society of Japan, Publications of the Astronomical Society of Japan},
 month = {},
 note = {application/pdf, High angular resolution near-infrared (JHK) adaptive optics images of T Tau were obtained with the infrared camera Coronagraphic Imager with Adaptive Optics (CIAO) mounted on the 8.2m Subaru Telescope in 2002 and 2004. The images resolve a complex circumstellar structure around a multiple system. We resolved T Tau Sa and Sb as well as T Tau N and S. The estimated orbit of T Tau Sb indicates that it is probably bound to T Tau Sa. The K band flux of T Tau S decreased by ˜ 1.7 Jy in 2002 November compared with that in 2001 mainly because T Tau Sa became fainter. The arc-like ridge detected in our near-infrared images is consistent with what is seen at visible wavelengths, supporting the interpretation in previous studies that the arc is part of the cavity wall seen relatively pole-on. Halo emission is detected out to ˜2''from T Tau N. This may be light scattered off the common envelope surrounding the T Tauri multiple system.},
 pages = {375--382},
 title = {Subaru near infrared coronagraphic images of T Tauri},
 volume = {58},
 year = {2006}
}