RADIO OBSERVATIONS OF PRE-PROTOSTARS

被引:6
作者
HUGHES, VA
机构
[1] Astronomy Group, Department of Physics, Queen's University, Kingston, Ont.
关键词
D O I
10.1038/222733a0
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
It is suggested that when an interstellar cloud, with associated magnetic field, collapses to form stars, the magnetic energy is dissipated in the acceleration of particles, producing non-thermal radio sources, and that the latter have been observed in the galactic plane. © 1969 Nature Publishing Group.
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页码:733 / &
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