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7篇 您的检索式：作者名="Chapillon"

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		题名	作者	年代	出处	被引量
	1	Effects of pre-and postnatal stimulation on developmental,emotional and cognitive aspects in rodents:a review显示文摘	Chapillon P Patin V Roy V	2002	Dev Psychobiol2002，41，4：	1
	2	Free versus forced exposure to an elevated plus-maze:evidence for new behavioral interpretations during test and retest显示文摘	Roy V Chapillon P Jeljeli M		0，，：	1
	3	Free versus forced exposure to an elevated plus-maze:evidence for new behavioral interpretations during test and retest显示文摘	Roy V Chapillon P Jeljeli M	2009	Psychopharmacology2009，203，1：	1
	4	Free versus forced exposure to an elevated plus-maze: evidence for new behavioral interpretations during test and retest显示文摘	Roy V Chapillon P Jeljeli M	2009	Psychopharmacology (Serl)2009，203，1：	1
	5	Free versus forced exposure toan elevated plus-maze:evidence for new behavioral interpretations during test and retest 显示文摘	Roy V Chapillon P Jeljeli M	2009	Psychopharmacology2009，203，1：	1
	6	Free versus forced exposure to an elevated plus-maze:evidence for new behavioral interpretations during test and retest显示文摘	Roy V Chapillon P Jeljeli M	2009	Psychopharmacology (Berl)2009，203，1：	1
	7	Morphology of the ^(13)CO(3–2) millimetre emission across the gas disc surrounding the triple protostar GG Tau A using ALMA observations显示文摘Observations by the Atacama Large Millimetre/sub-millimetre Array of the dust continuum and13 CO(3–2) millimetre emissions of the triple stellar system GG Tau A are analysed,giving evidence for a rotating gas disc and a concentric and coplanar dust ring. The present work complements an earlier analysis(Tang et al.) by exploring detailed properties of the gas disc. A 95% confidence level upper limit of 0.24′′(34 au) is placed on the disc scale height at a distance of 1′′(140 au) from the central stars. Evidence for Keplerian rotation of the gas disc is presented,with the rotation velocity reaching^3.1 km s^(-1) at 1′′ from the central stars,and a 99% confidence level upper limit of 9% is placed on relative contribution from a possible in-fall velocity. Variations of the intensity across the disc area are studied in detail and confirm the presence of a hot spot in the south-eastern quadrant. However several other significant intensity variations,in particular a depression in the northern direction,are also revealed. Variations of the intensity are found to be positively correlated to variations of the line width. Possible contributions to the measured line width are reviewed,suggesting an increase of the disc temperature and opacity with decreasing distance from the stars.	Nguyen Thi Phuong Pham Ngoc Diep Anne Dutrey Edwige Chapillon Pierre Darriulat Stéphane Guilloteau Do Thi Hoai Pham Tuyet Nhung Ya-Wen Tang Nguyen Thi Thao Pham Tuan-Anh	2018	Research in Astronomy and Astrophysics2018，18，3：	0

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