BRAINE, J.; GRATIER, P.; CONTRERAS, Y.; SCHUSTER, K. F.; BROUILLET, N.

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BRAINE, J.
FORMATION STELLAIRE 2012

GRATIER, P.
Institut de RadioAstronomie Millimétrique [IRAM]

CONTRERAS, Y.
Max-Planck-Institut für Radioastronomie [MPIFR]

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2012-10p. 89052

Resumen en inglés

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).< Leer menos

Palabras clave en inglés

Galaxies: nearby

Molecular clouds

Orígen

Importado de Hal

Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804