PROTOSTARS AS SOURCES OF ANOMALOUS OH EMISSION

被引：38

作者：

MEZGER, PG

ROBINSON, BJ

机构：

[1] National Radio Astronomy Observatory, Green Bank, WV

[2] Radiophysics Laboratory, CSIRO

来源：

NATURE | 1968年 / 220卷 / 5172期

关键词：

D O I：

10.1038/2201107a0

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：

Several lines of investigation suggest that the OH condensations are protostars associated with recently formed 0 stars. © 1968 Nature Publishing Group.

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页码：1107 / &

相关论文

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