PMO OpenIR
vycma水脉泽辐射的短时标变化
郑兴武1; 韩溥2; Eugenio Scalise Jr3
1997
Source Publication中国科学a辑数学
ISSN1006-9232
Volume027Issue:009Pages:858
Abstract利用紫金山天文台青海观测站的13.7m毫米波射电望远镜,在1993年8月26日 ̄9月24日的近1个月的时间里,每天监视大犬座VY(VY CMa)红超巨星拱星气体壳层中水脉泽辐射。发现一个强度相对变化为20% ̄25%,周期为10.3d的类正弦的快速振荡。这是迄今在红星中发现的变化周期最短的水脉泽辐射。给出了这个源的水分子脉泽谱线以及它的变化形态;利用细管状的完全饱和水脉泽辐射理论,估计了脉泽活动区的
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/29734
Collection中国科学院紫金山天文台
Affiliation1.南京大学
2.中国科学院紫金山天文台
3.Department of Astrophysics,INPE
Recommended Citation
GB/T 7714
郑兴武,韩溥,Eugenio Scalise Jr. vycma水脉泽辐射的短时标变化[J]. 中国科学a辑数学,1997,027(009):858.
APA 郑兴武,韩溥,&Eugenio Scalise Jr.(1997).vycma水脉泽辐射的短时标变化.中国科学a辑数学,027(009),858.
MLA 郑兴武,et al."vycma水脉泽辐射的短时标变化".中国科学a辑数学 027.009(1997):858.
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