THE DETECTION OF A NEW METHANOL MASER TRANSITION AT 9.9-GHZ

被引：11
|
作者：
SLYSH, VI
KALENSKII, SV
VALTTS, IE
机构：
[1] Astro-Space Center, Lebedev Physical Institute, Moscow 117810, Profsoyuznaya Street
来源：
ASTROPHYSICAL JOURNAL | 1993年 / 413卷 / 02期
关键词：
ISM; MOLECULES; MASERS; RADIO LINES; STARS; FORMATION;
D O I：
10.1086/186977
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A search for the 9(-1)-8(-2) E, 4(3)-5(2) A+, and 4(3)-5(2) A- methanol lines at 9.94, 9.98, and 10.06 GHz, respectively, was undertaken with the 43 m radio telescope at Green Bank. From a sample of 11 sources three were detected in emission for the 9(-1)-8(-2) E line, Orion-KL, Sgr B2, and W33-Met. The line in W33-Met shows maser properties; in Orion-KL and in Sgr B2 the line is thermal.
引用
收藏
页码：L133 / L135
页数：3
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