We present IRAM 30 m observations of the central ˜1.6 kpc of the spiral galaxy M81. 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.
Molecular Gas and Star Formation in M81
CASASOLA, VIVIANA;GALLETTA, GIUSEPPE;
2008
Abstract
We present IRAM 30 m observations of the central ˜1.6 kpc of the spiral galaxy M81. 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.File in questo prodotto:
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