Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...168..369i&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 168, no. 1-2, Nov. 1986, p. 369, 370.
Astronomy and Astrophysics
Astrophysics
16
Carbon Monoxide, Dwarf Galaxies, Emission Spectra, Irregular Galaxies, Molecular Clouds, Star Formation, Interstellar Gas, Star Formation Rate
Scientific paper
The authors searched for (1-0) 12CO emission in a sample of twelve irregular dwarf galaxies. The sample included galaxies with (U-V)0 colors at both the red and blue extremes, and thus presumably represented systems with both low and high star-formation rates. No emission was detected above (3σ) upper limits of about 25mK. The weak CO strength could be a consequence of a molecular hydrogen abundance lower than that in the Milky Way, or it could be due to the relatively low metal content in these small galaxies.
Burton William Butler
Israel Frank P.
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