The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136
David T. Frayer, Ronald J. Maddalena, R. J. Ivison, Ian Smail, Andrew, W. Blain, and Paul Vanden Bout

TL;DR
This study uncovers a previously unidentified massive molecular gas component in the archetypal submillimeter galaxy SMM J02399-0136, revealing complex gas dynamics and structures associated with galaxy mergers, outflows, or inflows at high redshift.
Contribution
It reports the discovery of a new extended molecular gas component W1 in SMM J02399-0136, characterized by lower excitation and significant mass, using combined GBT and ALMA observations.
Findings
Identification of a new molecular gas component W1
W1 accounts for about 30% of total molecular gas
W1 shows lower CO excitation than central regions
Abstract
We present CO(1-0), CO(3-2), and CO(7-6) observations using the Green Bank Telescope (GBT) and the Atacama Large Millimeter Array (ALMA) of the z=2.8 sub-millimeter galaxy SMM J02399-0136. This was the first submillimeter-selected galaxy discovered and remains an archetype of the class, comprising a merger of several massive and active components, including a quasar-luminosity AGN and a highly obscured, gas-rich starburst spread over a ~25 kpc extent. The GBT CO(1-0) line profile is comprised of two distinct velocity components separated by about 600 km/s and suggests the presence of a new component of molecular gas that had not been previously identified. The CO(3-2) observations with ALMA show that this new component, designated W1, is associated with a large extended structure stretching 13 kpc westward from the AGN. W1 is not detected in the ALMA CO(7-6) data implying that this gas…
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