Radio Observations of Pre-protostars

Details Radio Observations of Pre-protostars Radio Observations of Pre-protostars

May 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.222..733h&link_type=abstract

Nature, Volume 222, Issue 5195, pp. 733-735 (1969).

Physics

4

Scientific paper

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.

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