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Infrared characteristics of sources associated with OH, H2O, SiO and CH3OH masers

Published online by Cambridge University Press:  24 July 2012

Jarken Esimbek ,
Jian Jun. Zhou ,
Gang. Wu  and
Xin Di. Tang
Jarken Esimbek
Affiliation:
Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, PR China email: jarken@xao.ac.cn Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Urumqi 830011, PR China
Jian Jun. Zhou
Affiliation:
Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, PR China email: jarken@xao.ac.cn Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Urumqi 830011, PR China
Gang. Wu
Affiliation:
Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, PR China email: jarken@xao.ac.cn Key Laboratory of Radio Astronomy, Chinese Academy of Sciences, Urumqi 830011, PR China
Xin Di. Tang
Affiliation:
Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, PR China email: jarken@xao.ac.cn Graduate University of the Chinese Academy of Sciences, Beijing 100080, PR China
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Abstract

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We collect all published OH, H2O, SiO and CH3OH masers in the literature. The associated infrared sources of these four masers were identified with MSX PSC catalogues. We look for common infrared properties among the sources associated with four masers and make a statistical study. The MSX sources associated with stellar OH, stellar H2O and SiO masers concentrated in a small regions and the MSX sources associated with interstellar OH, interstellar H2O and CH3OH masers also concentrated in a small regions in an [A]-[D].vs.[A][-[E] diagram. These results give us new criterion to search for coexisting stellar maser samples for OH, H2O and SiO masers and interstellar maser samples for OH, H2O and CH3OH masers.

Keywords

MasersInterstellarStellarInfrared radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 178 - 179
Copyright
Copyright © International Astronomical Union 2012

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