Observations of stellar maser sources with no IRAS counterpart

被引:17
作者
Deguchi, S [1 ]
Nakashima, J
Miyata, T
Ita, Y
机构
[1] Grad Univ Adv Studies, Natl Astron Observ, Nobeyama Radio Observ, Nagano 3841305, Japan
[2] Grad Univ Adv Studies, Dept Astron Sci, Nagano 3841305, Japan
[3] Grad Univ Adv Studies, Dept Astron Sci, Nagano 3841305, Japan
[4] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
[5] Univ Tokyo, Inst Astron, Kiso Observ, Nagano 3970101, Japan
[6] Univ Tokyo, Inst Astron, Mitaka, Tokyo 1810015, Japan
关键词
masers; stars : AGB and post-AGB; stars : circumstellar matter; stars : late-type;
D O I
10.1093/pasj/57.6.933
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigated stellar maser sources with no IRAS counterpart at the radio, middle-infrared, and near-infrared wavelengths. A 43 GHz SiO maser search for 120 2MASS/MSX objects, and 10 OH 1612 MHz sources with no or a very faint MSX counterpart, resulted in 43 SiO detections: one OH 1612 MHz source, 2 near-infrared stars, and 40 MSX sources. Additional near-infrared J-, H-, and K-band observations of the OH 1612 MHz sources detected 5 near-infrared counterparts. Furthermore, middle-infrared imaging observations at 8.8, 9.7, 12.4, and 24.5 mu m with the Subaru 8.2-m telescope found counterparts for 2 near-infrared stars with SiO masers, and counterparts for 6 OH 1612 MHz sources. However, 4 OH 1612 MHz sources were not detected in the sensitive near- and middle-infrared searches; three of these are relatively strong OH maser sources for which the positions were known accurately. We conclude that one of these (OH 028.286-01.801) must be a young object in a star-forming region.
引用
收藏
页码:933 / 949
页数:17
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