NAOC Open IR
Distribution of SiO and OH Maser Stars in the Galactic Plane
Jiang Biwei; Jia Shumei
2001
Source PublicationChinese Journal of Astronomy and Astrophysics
ISSN1009-9271
Volume1Issue:2Pages:144
AbstractThe observational results of the Nobeyama 45-m SiO maser survey and the Arecibo 305-m OH maser survey are assembled for an analysis of the distribution and kinematics of late-type stars in the Galactic plane. It is found that neither SiO maser stars nor OH maser stars show any concentration to the spiral arms, which imply that they do not belong to the arm population and quite possibly they axe low-mass stars in late stage of evolution. A rotational curve is also derived for these objects and a few features which may be real are discussed and compared with those derived from planetary nebulae and AGB stars.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/39036
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Jiang Biwei,Jia Shumei. Distribution of SiO and OH Maser Stars in the Galactic Plane[J]. Chinese Journal of Astronomy and Astrophysics,2001,1(2):144.
APA Jiang Biwei,&Jia Shumei.(2001).Distribution of SiO and OH Maser Stars in the Galactic Plane.Chinese Journal of Astronomy and Astrophysics,1(2),144.
MLA Jiang Biwei,et al."Distribution of SiO and OH Maser Stars in the Galactic Plane".Chinese Journal of Astronomy and Astrophysics 1.2(2001):144.
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