The Water Vapor Spectrum of APM 08279+5255: X-Ray Heating and Infrared Pumping over Hundreds of Parsecs
C.M. Bradford, A.D. Bolatto, P.R. Maloney, J.E. Aguirre, J.J. Bock, J., Glenn, J. Kamenetzky, R. Lupu, H. Matsuhara, E.J. Murphy, B.J. Naylor, H.T., Nguyen, K. Scott, J. Zmuidzinas

TL;DR
This study analyzes the water vapor and CO spectra of quasar APM 08279+5255 at high redshift, revealing X-ray heating and infrared pumping effects that influence molecular excitation over hundreds of parsecs.
Contribution
First detection of multiple high-energy water transitions in a high-redshift quasar, demonstrating the role of X-ray heating and infrared pumping in molecular excitation.
Findings
CO cooling is consistent with an XDR model at 550-pc scale.
Water luminosity is comparable to CO, scaled up by a factor of 50.
High-lying water lines are excited radiatively by infrared pumping.
Abstract
We present the rest-frame 200--320 \mm\ spectrum of the z=3.91 quasar \apm, obtained with Z-Spec at the Caltech Submillimeter Observatory. In addition to the \jeight\ to \jthirteen\ CO rotational transitions which dominate the CO cooling, we find six transitions of water originating at energy levels ranging up to 643 K. Most are first detections at high redshift, and we have confirmed one transition with CARMA. The CO cooling is well-described by our XDR model, assuming L, and that the gas is distributed over a 550-pc sizescale, per the now-favored =4 lensing model. The total observed cooling in water corresponds to 6.5 \ls, comparable to that of CO. We compare the water spectrum with that of Mrk 231, finding that the intensity ratios among the high-lying lines are similar, but with a total luminosity scaled up by a…
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