High-ionization Fe K emission from luminous infrared galaxies

Details High-ionization Fe K emission from luminous infrared galaxies High-ionization Fe K emission from luminous infrared galaxies

2009-03-09

arxiv.org/abs/0903.1503v2

Astrophysical Journal, Letters 695, 103 (2009)

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

4 pages, 2 figures, ApJ Letters in press

Scientific paper

10.1088/0004-637X/695/1/L103

The Chandra component of the Great Observatories All-Sky LIRG Survey (GOALS) presently contains 44 luminous and ultraluminous infrared galaxies with log (Lir/Lsun) = 11.73-12.57. Omitting 15 obvious AGNs, the other galaxies are, on average, underluminous in the 2-10 keV band by 0.7 dex at a given far-infrared luminosity, compared to nearby star-forming galaxies with lower star formation rates. The integrated spectrum of these hard X-ray quiet galaxies shows strong high-ionization Fe K emission (Fe XXV at 6.7 keV), which is incompatible with X-ray binaries as its origin. The X-ray quietness and the Fe K feature could be explained by hot gas produced in a starburst, provided that the accompanying copious emission from high-mass X-ray binaries is somehow suppressed. Alternatively, these galaxies may contain deeply embedded supermassive black holes that power the bulk of their infrared luminosity and only faint photoionized gas is visible, as seen in some ULIRGs with Compton-thick AGN.

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