Molecular gas and star formation in M81
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🌌 astro-ph
keywords
molecularweakappearsbrightnesscentraldiscussemissionexcitation
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We present IRAM 30m observations of the central 1.6 kpc of the spiral M81 galaxy. The molecular gas appears weak and with an unusual excitation physics. We discuss a possible link between low CO emission and weak FUV surface brightness.
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