Radio observations of II ZW 40

Details Radio observations of II ZW 40 Radio observations of II ZW 40

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...224..808j&link_type=abstract

Astrophysical Journal, Part 1, vol. 224, Sept. 15, 1978, p. 808-811.

Astronomy and Astrophysics

Astronomy

27

Cosmic Dust, Galactic Structure, Interstellar Gas, Radio Astronomy, Balmer Series, H Ii Regions, H Lines, Infrared Astronomy, Interstellar Extinction

Scientific paper

Observations, using the Westerbork synthesis radio telescope at 21 cm in the line and at 6 cm in the continuum, of the dwarf galaxy II Zw 40 are presented. The continuum shows an infrared excess similar to the one found in galactic H II regions. A rough estimate based on the amount of internal absorption indicates a gas/dust ratio of the same order of magnitude as in our Galaxy, but observations in the far-infrared (100-300 microns) are needed to make better estimates.

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