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.
引用
收藏
页码：1107 / &
相关论文
共 26 条
[1]   OBSERVATIONS OF AN INFRARED STAR IN ORION NEBULA [J].
BECKLIN, EE ;
NEUGEBAUER, G .
ASTROPHYSICAL JOURNAL, 1967, 147 (02) :799-+
[2]   PRODUCTION OF OH MOLECULES IN INTERSTELLAR SHOCK WAVES [J].
FIELD, GB ;
AANNESTA.PA ;
SOLOMON, PM .
NATURE, 1968, 217 (5127) :435-&
[3]   THERMAL AND DYNAMICAL PROPERTIES OF A PROTOSTAR AND ITS CONTRACTION TO STAGE OF QUASI-STATIC EQUILIBRIUM [J].
HAYASHI, C ;
NAKANO, T .
PROGRESS OF THEORETICAL PHYSICS, 1965, 34 (05) :754-&
[4]   EVOLUTION OF PROTOSTARS [J].
HAYASHI, C .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1966, 4 :171-&
[5]   MECHANISM FOR ANOMALOUS OH EMISSION FROM H11 REGIONS [J].
HUGHES, VA .
NATURE, 1967, 215 (5104) :942-&
[6]   A MECHANISM FOR MASER ACTION OF OH MOLECULES IN INTERSTELLAR SPACE [J].
JOHNSTON, ID .
ASTROPHYSICAL JOURNAL, 1967, 150 (1P1) :33-&
[7]   DISCOVERY OF AN INFRARED NEBULA IN ORION [J].
KLEINMAN.DE ;
LOW, FJ .
ASTROPHYSICAL JOURNAL, 1967, 149 (1P2) :L1-&
[8]   OH OBSERVATIONS IN DIRECTIONS OF GALACTIC THERMAL SOURCES [J].
MCGEE, RX ;
GARDNER, FF ;
ROBINSON, BJ .
AUSTRALIAN JOURNAL OF PHYSICS, 1967, 20 (04) :407-&
[9]   GALACTIC H 2 REGIONS .2. OBSERVATIONS OF THEIR HYDROGEN 109ALPHA RECOMBINATION-LINE RADIATION AT FREQUENCY 5009 MHZ [J].
MEZGER, PG ;
HOGLUND, B .
ASTROPHYSICAL JOURNAL, 1967, 147 (02) :490-&
[10]   A NEW CLASS OF COMPACT H 2 REGIONS ASSOCIATED WITH ON EMISSION SOURCES [J].
MEZGER, PG ;
ALTENHOFF, W ;
SCHRAML, J ;
BURKE, BF ;
REIFENST.EC ;
WILSON, TL .
ASTROPHYSICAL JOURNAL, 1967, 150 (3P2) :L157-+
123