High-J v = SiS maser emission in IRC+10216:: A new case of infrared overlaps

被引:37
作者
Exposito, J. P. Fonfria [1 ]
Agundez, M. [1 ]
Tercero, B. [1 ]
Pardo, J. R. [1 ]
Cernicharo, J. [1 ]
机构
[1] Inst Estruct Mat, Dept Astrophys & Infrarroja, E-28006 Madrid, Spain
基金
美国国家科学基金会;
关键词
circumstellar matter; masers; stars : AGB and post-AGB; stars : carbon;
D O I
10.1086/507104
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the first detection of maser emission in the J = 11-10, J = 14-13, and J = 15-14 transitions of the p 0 vibrational state of SiS toward the carbon-rich star IRC + 10216. These masers seem to be produced v in the very inhomogeneous region between the star and the inner dust formation zone, located at similar or equal to(5-7)R-*, with expansion velocities below 10 km s(-1). We interpret the pumping mechanism as being due to overlaps between upsilon = 1-0 rovibrational lines of SiS and mid-IR lines of C2H2, HCN, and their C-13 isotopologues. The large number of overlaps found suggest the existence of strong masers for high-J upsilon = 0 and upsilon = 1 SiS transitions, located in the submillimeter range. In addition, it could be possible to find several rotational lines of the SiS isotopologues displaying maser emission.
引用
收藏
页码:L127 / L130
页数:4
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