Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004apjs..154..151s&link_type=abstract
The Astrophysical Journal Supplement Series, Volume 154, Issue 1, pp. 151-154.
Astronomy and Astrophysics
Astronomy
18
Galaxies: High-Redshift, Galaxies: Quasars: Emission Lines, Galaxies: Quasars: Individual: Alphanumeric: Apm 08279+5255, Techniques: Spectroscopic
Scientific paper
The Infrared Spectrograph (IRS) on board the Spitzer Space Telescope has been used to obtain low- and moderate-resolution spectra of the dust- and gas-rich quasar APM 08279+5255 (z=3.91). Broad Paα and Paβ recombination lines of hydrogen were detected at wavelengths of 9.235 and 6.315 μm, respectively, as well as a strong, red continuum that is a smooth power law over the observed (rest-frame) wavelength range 5.3-35 μm (1.08-7.1 μm). The observed Paα/Paβ line flux ratio of 1.05+/-0.2 is far from the case B value of ~2 and simple models of high-density, high optical depth ionized-gas regions (~1.8). This deviation is opposite in sense to the expected effect of reddening. No evidence is found in the spectrum for either the 3.3 or the 6.2 μm emission features usually attributed to aromatic hydrocarbons in gas-rich galaxies in the local universe. This is consistent with the high-luminosity active galactic nucleus (AGN) nature of APM 08279+5255.
The IRS was a collaborative venture between Cornell University and Ball Aerospace Corporation, funded by NASA through JPL and the Ames Research Center.
Appleton Phil N.
Armus Lee
Brandl Bernhard R.
Burgdorf Martin J.
Charmandaris Vassilios
No associations
LandOfFree
Spitzer Infrared Spectrograph (IRS) Observations of the Redshift 3.91 Quasar APM 08279+5255 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Spitzer Infrared Spectrograph (IRS) Observations of the Redshift 3.91 Quasar APM 08279+5255, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spitzer Infrared Spectrograph (IRS) Observations of the Redshift 3.91 Quasar APM 08279+5255 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1061722