Molecular gas and star formation in M81

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, 2 figures, to appear in "Pathways through an eclectic Universe", J. H. Knapen, T. J. Mahoney, and A. Vazdekis (Eds.),

Scientific paper

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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