Infrared observations of the radio source G30.8-0.0 in the W43 complex

Details Infrared observations of the radio source G30.8-0.0 in the W43 complex Infrared observations of the radio source G30.8-0.0 in the W43 complex

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193..283p&link_type=abstract

Astrophysical Journal, vol. 193, Oct. 1, 1974, pt. 1, p. 283-288.

Astronomy and Astrophysics

Astronomy

16

Cosmic Dust, Hydrogen Clouds, Infrared Astronomy, Nebulae, Radio Sources (Astronomy), Astronomical Maps, Brightness Temperature, Gas Ionization, Hydrogen Ions, Luminous Intensity, Point Sources

Scientific paper

Infrared observations of the G30.8-0.0 complex are presented. The data,
in conjunction with radio data on the same region, imply that dust may
be depleted within the region. The presence of an absorption feature at
10 microns is interpreted as due to a cool circumnebular cloud which
gives rise to the 100-micron intensity reported by airborne observers.

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