IRAS molecular clouds in the hot local interstellar medium.

Details IRAS molecular clouds in the hot local interstellar medium. IRAS molecular clouds in the hot local interstellar medium.

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988msngr..52...47a&link_type=abstract

The Messenger, vol. 52, p. 47-48

Physics

3

Interstellar Matter:Molecular Clouds, Molecular Clouds:Interstellar Matter

Scientific paper

The picture of the nearby (d <= 100 pC) interstellar medium, as resulting from the observations in the wavelength range from X-ray to radio, consists of a very hot, low-density gas, forming a hot bubble, filled with many cloudlets of ionized and neutral material and located near to an interstellar condensation (see the "Local Interstellar Medium", NASA CP-2345, 1984; and Cox and Reynolds, 1987).

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