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Luminous IR Galaxies in a Merger Sequence: BIMA CO Imaging

Yu Gao·R. A. Gruendl·C. -Y. Hwang·K. Y. Lo
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Abstract

In order to trace observationally the conditions in the interstellar medium (ISM) that lead to starbursts, we have used the newly expanded Berkeley-Illinois-Maryland Association (BIMA) millimeter-wave array to map the molecular ISM in a sample of LIGs chosen to represent different phases of the interacting/merging process. CO images of 6 galaxy mergers at the early/intermediate stage are shown here and preliminary results are summarized.

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Yu Gao, R. A. Gruendl, C. -Y. Hwang, K. Y. Lo. 1998-12-28. Luminous IR Galaxies in a Merger Sequence: BIMA CO Imaging. https://arxiv.org/abs/astro-ph/9812459

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