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		题名	作者	年代	出处	被引量
	1	Mono( imidazolin - 2- iminato) Titanium Complexes for EthylenePolymerization at Low Amounts of Methylaluminoxane显示文摘	Shoken D Sharma M Botoshansky M	2013	Journal of the American Chemical Society2013，135，12：	1
	2	Spaceborne coherent Doppler lidar显示文摘	Toshikazu I Shoken I	2002	Journal of the Communications Research Laboratory2002，49，2：	1
	3	Combined effects of selected food additives on adhesion of various foodborne pathogens onto microtiter plate and cabbage leaves显示文摘	Md Tariqul Islam Akinobu Oishi Chikako Machida Aya Ogura Shoken Kin Ken-ichi Honjoh Takahisa Miyamoto	2014	Food Control2014，，：	1
	4	Performance and Technique of Coherent 2-mm Differential Absorption and Wind Lidar for Wind Measurement显示文摘	Iwai Hironori Ishii Shoken Oda Ryoko Mizutani Kohei Sekizawa Shinya Murayama Yasuhiro	2013	Journal of Atmospheric and Oceanic Technology2013，，3：	1
	5	Human cardiac stem ceils exhibit mesenchymal features and are maintained through Akt/GSK - 3β signaling 显示文摘	Kento T Eishi A Shoken H	2007	Biochem Biophys Res Commun2007，352，：	1
	6	Near-infrared polarimetry of the GG Tauri A binary system显示文摘A high angular resolution near-infrared image that shows the intensity of polarization for the GG Tau A binary system was obtained with the Subaru Telescope.The image shows a circumbinary disk scattering the light from the central binary. The azimuthal profile of the intensity of polarization for the circumbinary disk is roughly reproduced by a simple disk model with the Henyey-Greenstein phase function and the Rayleigh function, indicating there are small dust grains at the surface of the disk.Combined with a previous observation of the circumbinary disk, our image indicates that the gap structure in the circumbinary disk orbits counterclockwise, but material in the disk orbits clockwise. We propose that there is a shadow caused by material located between the central binary and the circumbinary disk. The separations and position angles of the stellar components of the binary in the past 20 yr are consistent with the binary orbit with a = 33.4 AU and e = 0.34.	Yoichi Itoh Yumiko Oasa Tomoyuki Kudo Nobuhiko Kusakabe Jun Hashimoto Lyu Abe Wolfgang Brandner Timothy D.Brandt Joseph C.Carson Sebastian Egner Markus Feldt Carol A.Grady Olivier Guyon Yutaka Hayano Masahiko Hayashi Saeko S.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 H.Takahashi Naruhisa Takato Hiroshi Terada Christian Thalmann Daigo Tomono Edwin L.Turner Makoto Watanabe John Wisniewski Toru Yamada Satoshi Mayama Thayne Currie Hideki Takami Tomonori Usuda Motohide Tamura	2014	Research in Astronomy and Astrophysics2014，14，11：	0

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