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CO detections and IRAS observations of bright radio spiral galaxies at cz< or =9000 kilometers per second

Journal Article · · Astrophys. J., Lett. Ed.; (United States)
DOI:https://doi.org/10.1086/184561· OSTI ID:6077839
CO emission has been detected from 20 of 21 bright radio spirals with strong extended nuclear sources, including the most distant (NGC 7674) and the most luminous (IC 4553 = Arp 220, NGC 6240) galaxies yet detected in CO. All of these galaxies are rich in molecular gas, with M/sub total/(H2) = 3 x 10Y-2 x 10 M. IRAS observations show that they have a strong far-infrared (FIR) excess, with L/sub FIR//L/sub B/roughly-equal 1-35 and L/sub FIR/(40-400 m) roughly-equal 10 -10 S L. The primary luminosity source for these radio cores appears to be star formation in molecular clouds. A strong correlation is found between the FIR and extended 21 cm continuum flux, implying that the fraction of massive stars formed is independent of the star formation rate. The ratio L/sub FIR//M(H2) provides a measure of the current rate of star formation, which is found to be a factor 3-20 larger in these galaxies than for the ensemble of molecular clouds in the Milky Way. At these rates their molecular gas will be depleted in approx.10Y yr.
Research Organization:
Five College Radio Astronomy Observatory, University of Massachusetts; and California Institute of Technology
OSTI ID:
6077839
Journal Information:
Astrophys. J., Lett. Ed.; (United States), Journal Name: Astrophys. J., Lett. Ed.; (United States) Vol. 298:2; ISSN AJLEA
Country of Publication:
United States
Language:
English