SIMULTANEOUS OBSERVATIONS OF SiO AND H{sub 2}O MASERS TOWARD KNOWN STELLAR SiO AND H{sub 2}O MASER SOURCES. I
- Department of Astronomy and Space Science, Kyung Hee University, Seocheon-Dong, Giheung-Gu, Yongin, Gyeonggi-Do 446-701 (Korea, Republic of)
- Korean VLBI Network, Korea Astronomy and Space Science Institute, P.O. Box 88, Yonsei University, Seongsan-ro 262, Seodaemun, Seoul 120-749 (Korea, Republic of)
We present the results of simultaneous observations of both SiO and H{sub 2}O masers toward 166 known SiO and H{sub 2}O maser sources using the Korean VLBI Network Yonsei 21 m radio telescope during 2009 June. Both SiO and H{sub 2}O maser emission were detected from 112 sources giving a detection rate of 67% at one epoch observation. SiO-only maser emission was detected from 42 sources, while H{sub 2}O-only maser emission was detected from four sources. Most of the SiO masers appear around the stellar velocity, while H{sub 2}O masers show different characteristics compared with SiO masers. There are more than 20 sources that show a one-way peak or double peaks with respect to the stellar velocity and SiO maser peak velocity. The H{sub 2}O maser peak and integrated intensity ratios with respect to those of SiO (v = 1) show increasingly larger values from Mira variables, to OH/IR stars, to semi-regular variables. In addition, the IRAS two-color diagram of SiO and H{sub 2}O maser observational results is discussed.
- OSTI ID:
- 21454860
- Journal Information:
- Astrophysical Journal, Supplement Series, Vol. 188, Issue 1; Other Information: DOI: 10.1088/0067-0049/188/1/209; ISSN 0067-0049
- Country of Publication:
- United States
- Language:
- English
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COSMOLOGY AND ASTRONOMY
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ELECTRICAL EQUIPMENT
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HYDROGEN COMPOUNDS
MICROWAVE AMPLIFIERS
MICROWAVE EQUIPMENT
OXIDES
OXYGEN COMPOUNDS
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