Observation of the 12CO (J = 1→0) line in NGC 613 with the SEST.

Details Observation of the 12CO (J = 1→0) line in NGC 613 with the SEST. Observation of the 12CO (J = 1→0) line in NGC 613 with the SEST.

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989msngr..55...37b&link_type=abstract

The Messenger, vol. 55, p. 37-39

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1

Barred Spirals: Carbon Monoxide

Scientific paper

The availability of the Swedish-ESO SUbmillimeter Telescope (SEST) on La Silla opened the possibility of extending the radio observation of molecular lines to the very southern galaxies. In particular the observation of the CO lines in the nearest galaxies will permit not only to increase the sampling for statistical purposes but also to study in more detail the distribution and kinematical properties of the molecular clouds in relation to other components of the galaxies. The HPBW of the SEST, at the frequency of 115 GHz of the 12CO (J = 1 -> 0) line, is 43" which means that galaxies with diameters between 5.5 and 10 minutes of arc are weil suited for mapping since they do not require a prohibitive amount of time and the arms can be resolved if the inclination angle is adequate.

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