FURTHER MICROWAVE EMISSION LINES AND CLOUDS OF AMMONIA IN OUR GALAXY

被引：34

作者：

CHEUNG, AC

RANK, DM

TOWNES, CH

WELCH, WJ

机构：

[1] Radio Astronomy Laboratory, Department of Electrical Engineering, University of California

来源：

NATURE | 1969年 / 221卷 / 5184期

关键词：

D O I：

10.1038/221917a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Further NH3 emission has been found in the Sagittarius region, giving clues to the conditions in dust clouds. © 1969 Nature Publishing Group.

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页码：917 / &

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[1] DETECTION OF NH3 MOLECULES IN INTERSTELLAR MEDIUM BY THEIR MICROWAVE EMISSION
CHEUNG, AC
RANK, DM
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THORNTON, DD
WELCH, WJ
[J]. PHYSICAL REVIEW LETTERS, 1968, 21 (25) : 1701 - &
[2] DETECTION OF WATER IN INTERSTELLAR REGIONS BY ITS MICROWAVE RADIATION
CHEUNG, AC
RANK, DM
TOWNES, CH
THORNTON, DD
WELCH, WJ
[J]. NATURE, 1969, 221 (5181) : 626 - &