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Probing the origin of mass-loss in young T Tauri stars
Dougados, C; Lavalley, C; Cabrit, S
通讯作者Dougados, C
会议名称International Conference on Imaging the Universe in 3 Dimensions
会议日期MAR 29-APR 01, 1999
会议地点WALNUT CREEK, CA
英文摘要

We present spectre-imaging observations recently obtained with the TIGER and OASIS instruments at the CFHT, aimed at constraining the ejection and collimation mechanisms in active young premain sequence stars (age similar or equal to 1-3 Myrs). Three stars have been observed so far in the lines of [O I] 6300 Angstrom, H alpha, [N II] 6584 Angstrom and [S II] 6717,6731 Angstrom Angstrom with spatial resolutions ranging from 0.5 " to 0.25 " and velocity resolutions of 170 and 100 km s(-1). The morphology of the inner regions of the wind is revealed with unprecedented details. Constraints on excitation conditions and collimation and acceleration processes are derived.


来源出版物IMAGING THE UNIVERSE IN THREE DIMENSIONS: ASTROPHYSICS WITH ADVANCED MULTI-WAVELENGTH IMAGING DEVICES
出版年2000
卷号195
页码356-361
ISBN1-58381-022-6
出版者ASTRONOMICAL SOC PACIFIC
类型Proceedings Paper
语种英语
国家France
收录类别CPCI-S
WOS记录号WOS:000087281800048
WOS关键词DG-TAURI ; JETS ; ACCRETION ; LINE ; EMISSION ; OUTFLOWS ; STELLAR ; IMAGES
WOS类目Astronomy & Astrophysics
WOS研究方向Astronomy & Astrophysics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/293048
作者单位(1)Observ Grenoble, Astrophys Lab, F-38041 Grenoble 9, France
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Dougados, C,Lavalley, C,Cabrit, S. Probing the origin of mass-loss in young T Tauri stars[C]:ASTRONOMICAL SOC PACIFIC,2000:356-361.
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