High sensitivity SiO maser survey for mira variables |
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Authors: | Se-Hyung Cho Norio Kaifu Nobuharu Ukita Masaki Morimoto Masahiko Hayashi |
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Institution: | (1) Nobeyama Radio Observatory, Minamimaki, Nagano, Japan |
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Abstract: | Simultaneous observations of the six transitions of SiO for 106 late-type stars were made. The SiO maser emission was detected in 83 stars. Thev=3 maser emission was detected in eight stars, and the29SiOv=0 emission in six stars. The29SiOv=0 emission is stronger and narrower than that of28SiO, suggesting that the29SiO emission is masing.Paper presented at the IAU Third Asian-Pacific Regional Meeting, held in Kyoto, Japan, between 30 September–6 October, 1984. |
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