Astron. Astrophys. Suppl. Ser.
Volume 126, Number 1, November II 1997
|Page(s)||3 - 13|
|Published online||15 November 1997|
CO and H in a southern sample of interacting galaxies*
I. The data
Onsala Space Observatory, Chalmers University of Technology, S-439 92 Onsala, Sweden
Send offprint request to: C. Horellou
Accepted: 3 February 1997
Using SEST, the Parkes antenna and the Australia Telescope Compact Array, we have made a survey of the 12CO() and emission of an optically-selected sample of ≈ 60 southern interacting and merging galaxies. In this paper we present the data and determine global masses of neutral gas (in molecular and atomic form) for the observed galaxies. We have detected in 26 systems and found that these galaxies have less than 15% of their gas in molecular form.
Key words: galaxies: interaction / galaxies: ISM / galaxies / evolution / radio lines: galaxies
Figure 3 in its entirely is only available in electronic form at CDS via anonymous ftp to cdsarc.u-strasbg.fr (184.108.40.206) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1997