Free Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/201117056e]


Fig. A.1

thumbnail

CO(1–0) spectra for the galaxies detected with the IRAM 30 m telescope. The x-axis represents the recession velocity in  km s-1 and the y-axis the main beam brightness temperature Tmb in K. The spectral resolution is 20.8  km s-1 in most cases except for some individual galaxies for which a higher or lower resolution was required to clearly show the line. The full (red) line segment shows the line width of the CO line adopted for the determination of the velocity integrated intensity. The dashed (black) line segment is the HI line width at 20% peak level, W20. An asterisk next to the name indicates a marginal detection.

This figure is made of several images, please see below:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.