The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136
arXiv:1805.07212 · doi:10.3847/1538-4357/aac49a
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 has much lower CO excitation than the central starburst regions which are bright in CO(7-6). The molecular gas mass of W1 is about 30% of the total molecular gas mass in the system, depending on the CO--to--H_2 conversion factor. W1 is arguably a merger remnant; alternatively, it could be a massive molecular outflow associated with the AGN, or perhaps inflowing metal-enriched molecular gas fueling the ongoing activity.
10 pages, 8 figures. Accepted for publication in ApJ 2018.05.11
References in corpus (16)
- The Frontier Fields: Survey Design
- Intense Star Formation within Resolved Compact Regions in a Galaxy at z=2.3
- The Green Bank Ammonia Survey (GAS): First Results of NH3 mapping the Gould Belt
- Molecular Gas in the Halo Fuels the Growth of a Massive Cluster Galaxy at High Redshift
- The Role of Galactic Winds on Molecular Gas Emission from Galaxy Mergers
- Molecular gas in low-metallicity starburst galaxies: Scaling relations and the CO-to-H conversion factor
- Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
- A Survey of the Molecular ISM Properties of Nearby Galaxies using the Herschel FTS
- High-J CO SLEDs in nearby infrared bright galaxies observed by Herschel-PACS
- Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [CI]
- First Detection of the [OIII] 88 micron Line at High Redshifts: Characterizing the Starburst and Narrow Line Regions in Extreme Luminosity Systems
- Observing Cold Gas in Submillimeter Galaxies: Detection of CO(1-0) Emission in SMM J13120+4242 with the Green Bank Telescope
- VLA imaging of 12CO J=1-0 and free-free emission in lensed submillimetre galaxies
- Physical conditions of molecular gas in the Circinus galaxy: Multi-J CO and CI 1-0 observations
- Total Molecular Gas Masses of Planck - Herschel Selected Strongly Lensed Hyper Luminous Infrared Galaxies
- The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
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- VLA-ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): Total Cold Gas Masses and CO Line Ratios for z=2-3 "Main Sequence" Galaxies
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- VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
- The cold circumgalactic environment of MAMMOTH-I: dynamically cold gas in the core of an Enormous Ly-alpha Nebula
- The ALMA-CRISTAL survey. Discovery of a 15 kpc-long gas plume in a Lyman- blob
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