A Survey of YSOs with Micro-Jets
A Survey of YSOs with Micro-Jets
批准号:
11640238
负责人:
SUGITANI Koji
金额:
$1.6万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for Scientific Research (C)
财政年份:
1999
资助国家:
日本
项目状态:
已结题
起止时间:
1999 至 2000
中文摘要
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英文摘要
The acceleration and collimation of high-velocity jets associated with YSOs (Young Stellar Objects) are considered to be deeply related to their circumstellar disks. In this research, through observations of near-infrared and optical observation as well as X-ray and radio, we aimed to search for target candidates for detailed studies of the jets, micro-jets and circumstellar disks with Subaru Telescope and/or other large telescopes.We have analyzed the low-dispersion grism spectroscopy data which we obtained with the 2.2m telescope of University of Hawaii and 2.6m telescope of Byurakan Astrophysical Observatory in 1999. As a result, we identified about 10 H alpha stars in star forming regions very near to the sun and many H alpha stars toward the HII regions with bright-rimmed clouds, which are good candidates of YSOs having micro-jects and/or cicumstellar disks. We made followup observations for some of the above candidates by using HARIS (High Angular Resolution Imaging Spectrograph) of University of Hawaii. The lithium absorption line, which is a good indicator of YSO, was detected in most of them. We also obtained near-infrared data for these objects by using SIRIUS (simultaneously Infrared Imager for Unbiased Survey). In the southern sky, we started to search for H alpha stars in nearby star forming regions in the southern sky.
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K.Sugitani,M.Tamura,K.Ogura: "Small-Scale Sequential Star Formation in Bright-Rimmed Clouds"Star Formation 1999,Proceedings of Star Formation 1999,held in Nagoya,Japan ,June 21-25,1999,Editor:T.Nakamoto,Nobeyama Radio Observatory. 358-364 (1999)
K.Sugitani,M.Tamura,K.Ogura:“Small-Scale Sequential Star Formation in Bright-Rimmed Clouds”Star Formation 1999,Proceedings of Star Formation 1999,于日本名古屋举行,1999年6月21-25日,编辑:
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K.Ogura,K.Sugitani: "A Large Number of Hα; Emission Stars Associated with Bright-Rimmed Clouds"Star Formation 1999,Proceedings of Star Formation 1999,held in Nagoya,Japan ,June 21-25,1999,Editor:T.Nakamoto,Nobeyama Radio Observatory. 381-382 (1999)
K.Ogura、K.Sugitani:“A Large Number of Hα; Emission Stars Associated with Bright-Rimmed Clouds”Star Formation 1999,Proceedings of Star Formation 1999,于日本名古屋举行,1999 年 6 月 21-25 日,编辑:T .Nakamoto,野边山无线电天文台。381-382(1999)
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Nakano,M.Yamauchi,S.,Sugitani,K.,Ogura,K.: "ASCA Observations of the NGC 2264 Molecular Cloud"Astronomical Society of Japan. 52. 437-446 (2000)
Nakano,M.Yamauchi,S.、Sugitani,K.、Ogura,K.:“NGC 2264 分子云的 ASCA 观测”日本天文学会。
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Mikami,T.Ogura,K.: "Hα Emission Stars in the Cepheus OB3 Region"Astrophysics and Space Science. 275. 441-462 (2001)
Mikami, T. Ogura, K.:“仙王座 OB3 区域的 Hα 发射星”天体物理学和空间科学 275. 441-462 (2001)。
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K.Sugitani,et al.: "2 Millimeter Observations of Bright-rimmed Clouds with IRAS Point Sources"Astrophysical Journal. 119. 323-334 (2000)
K.Sugitani 等人:“用 IRAS 点源对亮边云进行 2 毫米观测”天体物理学杂志。
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Studies of Magnetic Field Structures in Infrared Dark Clouds
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批准号:24540233
-
项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$3.24万
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财政年份:2012
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负责人:SUGITANI Koji
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依托单位:
A large-scale search for T Tauri stars toward star cluster forming regions
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批准号:20403003
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项目类别:Grant-in-Aid for Scientific Research (B)
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资助金额:$9.4万
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财政年份:2008
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负责人:SUGITANI Koji
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依托单位:
A Search for T Tauri Stars toward Dense Cores
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批准号:19540242
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项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$2.91万
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财政年份:2007
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负责人:SUGITANI Koji
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依托单位:
A survey of T Tauri stars in the nearest star forming regions
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批准号:14540228
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项目类别:Grant-in-Aid for Scientific Research (C)
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资助金额:$2.05万
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财政年份:2002
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负责人:SUGITANI Koji
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依托单位:
国内基金
海外基金
Accretion variability and its consequences: from protostars to planet-forming disks
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批准号:12173003
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项目类别:面上项目
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资助金额:60万元
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批准年份:2021
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负责人:沈雷歌
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依托单位: