Time variations of water vapor masers in star-forming regions

被引：0
|
作者：
MendozaTorres, JE
Lekht, EE
机构：
来源：
STAR FORMATION NEAR AND FAR - SEVENTH ASTROPHYSICS CONFERENCE | 1997年 / 393期
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The results of observations of water vapor maser at 22.2 GHz made during of about 15 years are presented. The results show that anticorrelation between the fluxes of different spectral ranges as well as of different spectral features is a common phenomenon in Star-Forming Regions (SFR) masers. We interpret these results as indicating that partial saturation commonly occurs in SFR water vapor masers.
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页码：197 / 200
页数：4
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