4.6 Article

Cold dust and molecular gas towards the centers of Magellanic type galaxies and irregulars - I. The data

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ASTRONOMY & ASTROPHYSICS
卷 414, 期 1, 页码 141-U10

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DOI: 10.1051/0004-6361:20031634

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galaxies : interstellar matter; galaxies : abundances; galaxies : Magellanic type; radio lines : galaxies; radio continuum : galaxies

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We present 1300 mum continuum emission measurements and observations of the (CO)-C-12 (1-0) and (2-1) transition towards the centers of 64 Magellanic type galaxies (Sdm/Sm) and irregulars (Im/I0/Irr). The sources are selected to have IRAS flux densities S(100 mum)greater than or equal to1000 mJy and optical diameters mainly below 180. We were able to detect (CO)-C-12 towards 41 and the continuum emission towards 28 galaxies. In addition, we obtained the corresponding data for a set of 6 complementary galaxies of different morphological type.

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