DISCOVERY OF WATER VAPOR IN THE HIGH-REDSHIFT QUASAR APM 08279+5255 AT z = 3.91
Journal Article
·
· Astrophysical Journal Letters
- California Institute of Technology, Cahill Center for Astronomy and Astrophysics 301-17, Pasadena, CA 91125 (United States)
- Department of Physics and Astronomy, The Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States)
- LERMA, UMR 8112 du CNRS, Observatoire de Paris and Ecole Normale Superieure, 24 Rue Lhomond, 75231 Paris cedex 05 (France)
- IRAM-Institut de Radio Astronomie Millimetrique, 300 rue de la Piscine, 38406 Saint-Martin d'Heres (France)
We report a detection of the excited 2{sub 20}-2{sub 11} rotational transition of para-H{sub 2}O 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 large velocity gradient 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 hydrogen fluoride (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 interstellar medium.
- OSTI ID:
- 21562450
- Journal Information:
- Astrophysical Journal Letters, Journal Name: Astrophysical Journal Letters Journal Issue: 1 Vol. 738; ISSN 2041-8205
- Country of Publication:
- United States
- Language:
- English
Similar Records
THE WATER VAPOR SPECTRUM OF APM 08279+5255: X-RAY HEATING AND INFRARED PUMPING OVER HUNDREDS OF PARSECS
A STUDY OF THE X-RAYED OUTFLOW OF APM 08279+5255 THROUGH PHOTOIONIZATION CODES
AKARI NEAR- AND MID-INFRARED SPECTROSCOPY OF APM 08279+5255 AT z = 3.91
Journal Article
·
Wed Nov 09 23:00:00 EST 2011
· Astrophysical Journal Letters
·
OSTI ID:22047366
A STUDY OF THE X-RAYED OUTFLOW OF APM 08279+5255 THROUGH PHOTOIONIZATION CODES
Journal Article
·
Sat Aug 20 00:00:00 EDT 2011
· Astrophysical Journal
·
OSTI ID:21579934
AKARI NEAR- AND MID-INFRARED SPECTROSCOPY OF APM 08279+5255 AT z = 3.91
Journal Article
·
Wed May 20 00:00:00 EDT 2009
· Astrophysical Journal
·
OSTI ID:21300588