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Autre Publication Scientifique Année : 2012

Molecular cloud formation in M 33 (Braine+, 2012)

Résumé

The amount of H2 present in spiral galaxies remains unce particularly in the dim outer regions and in low-metallicity environments. We present high-resolution CO(1-0) observations with the Plateau de Bure interferometer of the most distant molecular cloud in the local group galaxy M33. The cloud is a single entity rather than a set of smaller clouds within the broad beam of the original single-dish observations. The interferometer and single-dish fluxes are very similar and the line widths are indistinguishable, despite the difference in beamsize. (2 data files).
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Dates et versions

hal-00787032 , version 1 (11-02-2013)

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J. Braine, P. Gratier, Y. Contreras, K. F. Schuster, N. Brouillet. Molecular cloud formation in M 33 (Braine+, 2012). 2012, pp.89052. ⟨hal-00787032⟩
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