Astronomy and Astrophysics – Astronomy
Scientific paper
May 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...197l..22k&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 197, no. 1-2, May 1988, p. L22-L24. Research supported by the Japan Society fo
Astronomy and Astrophysics
Astronomy
2
Active Galactic Nuclei, Galaxies, Hydroxyl Emission, Interstellar Matter, Peculiar Galaxies, Star Formation, Infrared Astronomy Satellite, Molecular Clouds, Morphology, Stellar Luminosity
Scientific paper
Observations of IC 860 in CO (lambda = 2.6 mm) have been compared to existing data in HI (lambda = 21 cm) and OH (lambda = 18 m). The present measured central velocity of 3933 km/s for CO is found to be close to those measured for HI and OH. The results are consistent with a disk, or possibly spiral, morphology for IC 860. The star formation efficiency of the object is considered, and it is suggested that IC 860 behaves both like an interacting and a starburst galaxy.
Handa Toshihiro
Karoji Hiroshi
Kazes Ilya
Nakai Noriyuki
Sofue Yoshiaki
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