Discovery of Water Vapor in the High-Redshift Quasar APM 08279+5255 at Z=3.91
arXiv:1106.4784 · doi:10.1088/2041-8205/738/1/L6
Abstract
We report a detection of the excited 220-211 rotational transition of para-H2O in APM 08279+5255 using the IRAM Plateau de Bure interferometer. At z = 3.91, this is the highest-redshift detection of interstellar water to date. From LVG modeling, we conclude that this transition is predominantly radiatively pumped and on its own does not provide a good estimate of the water abundance. However, additional water transitions are predicted to be detectable in this source, which would lead to an improved excitation model. We also present a sensitive upper limit for the HF J = 1 - 0 absorption toward APM 08279+5255. While the face-on geometry of this source is not favorable for absorption studies, the lack of HF absorption is still puzzling and may be indicative of a lower fluorine abundance at z = 3.91 compared with the Galactic ISM.
5 pages, 2 figures, to appear in The Astrophysical Journal Letters
References in corpus (6)
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Cited by in corpus (19)
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- Submillimeter H2O and H2O+ emission in lensed ultra- and hyper-luminous infrared galaxies at z ~ 2-4
- Water vapor emission reveals a highly obscured, star forming nuclear region in the QSO host galaxy APM08279+5255 at z=3.9
- Modeling the H2O submillimeter emission in extragalactic sources
- An ALMA Early Science survey of molecular absorption lines toward PKS1830-211 -- Analysis of the absorption profiles
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- Gravitational lensing reveals extreme dust-obscured star formation in quasar host galaxies
- The Water Vapor Spectrum of APM 08279+5255: X-Ray Heating and Infrared Pumping over Hundreds of Parsecs
- A proto-pseudobulge in ESO 320-G030 fed by a massive molecular inflow driven by a nuclear bar
- Discovery of Hydrogen Fluoride in the Cloverleaf Quasar at z = 2.56
- Stacked Average Far-Infrared Spectrum of Dusty Star-Forming Galaxies from the Herschel/SPIRE Fourier Transform Spectrometer
- SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys
- Unveiling the warm dense ISM in quasar host galaxies via water vapor emission
- Detection of H2O and OH+ in z>3 Hot Dust-Obscured Galaxies
- Etching glass in the early Universe: Luminous HF and water emission in a QSO-SMG pair at z=4.7
- Constraining the Active Galactic Nucleus and Starburst Properties of the IR-luminous Quasar Host Galaxy APM 08279+5255 at Redshift 4 with SOFIA
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