Radio observations of bright ionized rims

Details Radio observations of bright ionized rims Radio observations of bright ionized rims

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...298..292s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 298, Nov. 1, 1985, p. 292-295.

Astronomy and Astrophysics

Astronomy

12

Hydrogen Clouds, Interstellar Gas, Ionized Gases, Molecular Clouds, Radio Sources (Astronomy), Condensation, Nebulae, Neutral Gases, Taylor Instability

Scientific paper

Radio images of ionized bright rim structures in NGC 2264, IC 1396, and
S 140 show discrete condensations which are not optically evident. These
condensations may be the result of Rayleigh-Taylor instabilities at the
interface between the ionized and neutral phases of the interstellar
medium.

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