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A possible origin of 6.7 GHz linear methanol maser sources
Xu, Y1,2,3
2001-10-01
Source PublicationCHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
ISSN1009-9271
Volume1Issue:5Pages:389-394
Contribution Rank2
Abstract

We present a model which explains the observed multi-linear spatial structures with different velocity gradients of the 5(0)-6(1)A(+) methanol line at 6.7 GHz. We consider this and other hypotheses and conclude that the methanol maser emission probably comes from some thin rings variously inclined to the line of sight.

KeywordMasers Stars : Circumstellar Matter Stars : Formation
SubtypeArticle
Subject Area恒星和恒星物理
WOS HeadingsScience & Technology ; Physical Sciences
URL查看原文
Indexed BySCI
Language英语
WOS KeywordStar-forming Regions ; H-ii Regions ; Vlbi Observations ; Iras Sources ; Disks ; Discovery ; W3(Oh) ; Galaxy ; Search ; Flare
Funding Project恒星形成与演化研究团组
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000172419200002
Funding Organization国家自然科学基金
Citation statistics
Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/38
Collection射电天文研究室_恒星形成与演化研究团组
Corresponding AuthorXu, Y
Affiliation1.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Urumqi Astron Observ, Urumqi 830011, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Xu, Y. A possible origin of 6.7 GHz linear methanol maser sources[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2001,1(5):389-394.
APA Xu, Y.(2001).A possible origin of 6.7 GHz linear methanol maser sources.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,1(5),389-394.
MLA Xu, Y."A possible origin of 6.7 GHz linear methanol maser sources".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 1.5(2001):389-394.
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