中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The discovery based on GLIMPSE data of a protostar driving a bipolar outflow (Research Note)

文献类型:期刊论文

作者Yuan, Jing-Hua1; Li, Jin Zeng1; Huang, Ya Fang1; Hsia, Chih-Hao2; Miao, Jingqi3
刊名ASTRONOMY & ASTROPHYSICS
出版日期2012-04-01
卷号540
关键词ISM: jets and outflows stars: early-type stars: formation stars: protostars
英文摘要We report the discovery based on GLIMPSE data of a proto-stellar system driving a bipolar outflow. The bipolar outflow closely resembles the shape of an hourglass in the infrared. The total luminosity of L-total = 5507 L-circle dot, derived from IRAS fluxes, indicates the ongoing formation of a massive star in this region. The spectral energy distribution (SED) of the driving source is fitted with an online SED fitting tool, which results in a spectral index of about 1.2. This, along with the presence of a bipolar outflow, suggests the detection of a Class I protostar. The driving source indicates prominent infrared excesses in color-color diagrams based on archived 2MASS and GLIMPSE data, which is in line with an early evolutionary stage of the system.
收录类别SCI
语种英语
WOS记录号WOS:000303315400109
源URL[http://ir.bao.ac.cn/handle/114a11/6319]  
专题国家天文台_应用天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China
3.Univ Kent, Ctr Astrophys & Planetary Sci, Sch Phys Sci, Canterbury CT2 7NR, Kent, England
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GB/T 7714
Yuan, Jing-Hua,Li, Jin Zeng,Huang, Ya Fang,et al. The discovery based on GLIMPSE data of a protostar driving a bipolar outflow (Research Note)[J]. ASTRONOMY & ASTROPHYSICS,2012,540.
APA Yuan, Jing-Hua,Li, Jin Zeng,Huang, Ya Fang,Hsia, Chih-Hao,&Miao, Jingqi.(2012).The discovery based on GLIMPSE data of a protostar driving a bipolar outflow (Research Note).ASTRONOMY & ASTROPHYSICS,540.
MLA Yuan, Jing-Hua,et al."The discovery based on GLIMPSE data of a protostar driving a bipolar outflow (Research Note)".ASTRONOMY & ASTROPHYSICS 540(2012).

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来源:国家天文台

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