| Issue |
A&A
Volume 414, Number 1, January IV 2004
|
|
|---|---|---|
| Page(s) | 141 - 153 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361:20031634 | |
| Published online | 12 January 2004 | |
Cold dust and molecular gas towards the centers of Magellanic type galaxies and irregulars *,**
I. The data
1
Astronomisches Institut der Ruhr-Universität Bochum, Universitätsstr. 150, 44780 Bochum, Germany e-mail: albrecht@astro.rub.de
2
Max Planck Institut für Radioastronomie Bonn, Auf dem Hügel 69, 53121 Bonn, Germany
Corresponding author: M. Albrecht, albrecht@astro.rub.de
Received:
29
July
2003
Accepted:
16
October
2003
We present 1300 μm continuum emission measurements and
observations of the ![$\element[][12]{CO}$](/articles/aa/abs/2004/04/aah4699/aah4699_tex_eq1.png)
(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
mJy and optical diameters mainly below 180´´.
We were able to detect 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.
Key words: galaxies: interstellar matter / galaxies: abundances / galaxies: Magellanic type / radio lines: galaxies / radio continuum: galaxies
© ESO, 2004
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