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http://hdl.handle.net/20.500.12386/26268
Title: | New Constraints on the Molecular Gas in the Prototypical HyLIRGs BRI1202-0725 and BRI1335-0417 | Authors: | Jones, G. C. Carilli, C. L. Momjian, E. Wagg, J. Riechers, D. A. Walter, F. DECARLI, ROBERTO Ota, K. McMahon, R. |
Issue Date: | 2016 | Journal: | THE ASTROPHYSICAL JOURNAL | Number: | 830 | Issue: | 2 | First Page: | 63 | Abstract: | We present Karl G Jansky Very Large Array observations of CO(J=2\to 1) line emission and rest-frame 250 GHz continuum emission of the Hyper-Luminous IR Galaxies (HyLIRGs) BRI 1202-0725 (z = 4.69) and BRI 1335-0417 (z = 4.41), with an angular resolution as high as 0.″15. Our low-order CO observations delineate the cool molecular gas, the fuel for star formation in the systems, in unprecedented detail. For BRI 1202-0725, line emission is seen from both extreme starburst galaxies: the quasar host and the optically obscured submm galaxy (SMG), in addition to one of the Lyα emitting galaxies in the group. Line emission from the SMG shows an east-west extension of about 0.″6. For Lyα-2, the CO emission is detected at the same velocity as [C II] and [N II], indicating a total gas mass ∼4.0 × 10<SUP>10</SUP> M <SUB>☉</SUB>. The CO emission from BRI 1335-0417 peaks at the nominal quasar position, with a prominent northern extension (∼1″, a possible tidal feature). The gas depletion timescales are ∼10<SUP>7</SUP> years for the three HyLIRGs, consistent with extreme starbursts, while that of Lyα-2 may be consistent with main sequence galaxies. We interpret these sources as major star formation episodes in the formation of massive galaxies and supermassive black holes via gas-rich mergers in the early universe. | URI: | http://hdl.handle.net/20.500.12386/26268 | URL: | https://iopscience.iop.org/article/10.3847/0004-637X/830/2/63 | ISSN: | 0004-637X | DOI: | 10.3847/0004-637X/830/2/63 | Bibcode ADS: | 2016ApJ...830...63J | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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Jones_2016_ApJ_830_63.pdf | Pdf editoriale | 4.55 MB | Adobe PDF | View/Open |
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