CO Emission in Low-Luminosity, H I-rich Galaxies

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© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Christopher L. Taylor et al 1998 AJ 116 2746 DOI 10.1086/300655

1538-3881/116/6/2746

Abstract

     We combine these new observations with data from the literature to form a sample of dwarf galaxies that all have CO observations and measured oxygen abundances. No known galaxies with 12 + log (O/H) < 7.9 (Z < 0.1 Z) have been detected in CO. Most of the star-forming galaxies with higher [12 + log (O/H) > 8.1] metallicities are detected at similar or higher ICO surface brightnesses. The data are consistent with a strong dependence of the ICO/MXCO conversion factor on ambient metallicity. The strikingly low upper limits on some metal-poor galaxies lead us to predict that the conversion factor is nonlinear, increasing sharply below ∼1/10 of the solar metallicity [12 + log (O/H) ≤ 7.9].

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10.1086/300655