Journal
ASTROPHYSICAL JOURNAL
Volume 549, Issue 2, Pages L191-L194Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/319175
Keywords
galaxies : general; galaxies : ISM; galaxies : spiral; ISM : molecules
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We have obtained deep CO (1-0) observations of eight nearby, edge-on, low surface brightness (LSB) spiral galaxies using the NRAO 12 m telescope. We report detections of three of our targets at a greater than 4 sigma level as well as one marginal (similar to3 sigma) detection. These are among the first direct detections of molecular gas in late-type, LSB spiral galaxies. Using a Galactic CO-to-H-2 conversion factor, we derive M-H2 similar to (1.4-3.5) x 10(7) M. and M-H2/M-H1 similar to 0.010-0.055 for the detected sources, with 3 sigma upper limits of M-H2 less than or equal to (0.7-5 7) x 10(7) M. and M-H2/M-H1 less than or similar to 0.006-0.029 for the undetected objects.
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