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arXiv · 0706.3769

Molecular gas and star formation in M81

V. Casasola·F. Combes·G. Galletta·D. Bettoni
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Abstract

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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V. Casasola, F. Combes, G. Galletta, D. Bettoni. 2007-06-26. Molecular gas and star formation in M81. https://arxiv.org/abs/0706.3769

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