Molecular gas and star formation in M81

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dc.creatorCasasola, V.
dc.creatorCombes, F.
dc.creatorGalletta, G.
dc.creatorBettoni, D.
dc.date2007-06-26
dc.date.accessioned2026-07-07T08:12:25Z
dc.date.available2026-07-07T08:12:25Z
dc.descriptionWe 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.
dc.description2 pages, 2 figures, to appear in "Pathways through an eclectic Universe", J. H. Knapen, T. J. Mahoney, and A. Vazdekis (Eds.), ASP Conf. Ser., 2007
dc.identifierhttps://arxiv.org/abs/0706.3769
dc.identifierhttp://arxiv.org/abs/0706.3769
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/132449
dc.subjectAstrophysics
dc.titleMolecular gas and star formation in M81
dc.typetext

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