Evolution of the H2O maser emission in IRAS 20126+4104

被引：0
|
作者：
Lekht, E. E. [1 ]
Pashchenko, M. I. [1 ]
Rudnitskii, G. M. [1 ]
机构：
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2015年 / 41卷 / 11期
基金：
俄罗斯基础研究基金会;
关键词：
star formation; masers; jets and flows; individual objects (IRAS 20126+4104); IRAS-20126+4104; RESOLUTION; OUTFLOW; DISK; JET;
D O I：
10.1134/S1063773715100035
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the results of our investigation of the H2O maser emission from individual features in IRAS 20126+4104, which is a cold infrared source. The observations were performed at the 22-m radio telescope of the Pushchino Radio Astronomy Observatory. A radial-velocity drift of the features caused by their deceleration at the interface between between an accelerated jet and the surrounding molecular environment has been detected. The observed tendency for the H2O emission as a whole to drift is associated with the successive excitation of maser features or their clusters by the front of a shock (or magnetohydrodynamic) wave. An estimate of the jet rotation period is provided (similar to 150 years).
引用
收藏
页码：607 / 612
页数：6
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