DISCOVERY OF HYDROXYL RADIO EMISSION FROM INFRARED STARS

被引：122

作者：

WILSON, WJ

BARRETT, AH

机构：

来源：

SCIENCE | 1968年 / 161卷 / 3843期

关键词：

D O I：

10.1126/science.161.3843.778

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：

Radio spectral line emission from hydroxyl radicals has been detected from four infrared stars. The emission from the infrared star NML Cygni at 1612 megahertz is the strongest radio emission line yet detected. Sixteen other stars with infrared excesses showed no detectable hydroxyl radio emission.

引用

页码：778 / &

共 15 条

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