AN INTERFEROMETRIC SPECTRAL-LINE SURVEY OF IRC+10216 IN THE 345 GHz BAND

被引:59
作者
Patel, Nimesh A. [1 ]
Young, Ken H. [1 ]
Gottlieb, Carl A. [1 ]
Thaddeus, Patrick [1 ]
Wilson, Robert W. [1 ]
Menten, Karl M. [2 ]
Reid, Mark J. [1 ]
McCarthy, Michael C. [1 ]
Cernicharo, Jose [3 ]
He, Jinhua [4 ]
Bruenken, Sandra [5 ]
Dinh-V. Trung [6 ]
Keto, Eric [1 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Max Planck Inst Radioastron, D-53121 Bonn, Germany
[3] INTA CSIC, Lab Mol Astrophys, Dept Astrophys, CAB, Madrid 28850, Spain
[4] Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China
[5] Univ Cologne, Inst Phys 1, D-50937 Cologne, Germany
[6] Acad Sinica, Inst Astron & Astrophys, Taipei 106, Taiwan
关键词
astrochemistry; line: identification; stars: AGB and post-AGB; stars:; individual; (IRC+10216; CW Leo); surveys; GIANT BRANCH STARS; SUBMILLIMETER OBSERVATIONS; CIRCUMSTELLAR ENVELOPE; MOLECULAR-SPECTROSCOPY; COLOGNE DATABASE; EVOLVED STARS; CARBON STAR; IRC +10216; EMISSION; MILLIMETER;
D O I
10.1088/0067-0049/193/1/17
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report a spectral-line survey of the extreme carbon star IRC+10216 carried out between 293.9 and 354.8 GHz with the Submillimeter Array. A total of 442 lines were detected, more than 200 for the first time; 149 are unassigned. Maps at an angular resolution of similar to 3 '' were obtained for each line. A substantial new population of narrow lines with an expansion velocity of similar to 4 km s(-1) (i.e., approximate to 30% of the terminal velocity) was detected. Most of these are attributed to rotational transitions within vibrationally excited states, emitted from energy levels above the v = 0, J = 0 ground state with excitation energy of 1000-3000 K. Emission from these lines appears to be centered on the star with an angular extent of < 1 ''. We use multiple transitions detected in several molecules to derive physical conditions in this inner envelope of IRC+10216.
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页数:65
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