CaltechAUTHORS
  A Caltech Library Service

Subarcsecond Mid-Infrared Observations of NGC 6240: Limitations of Active Galactic Nucleus-Starburst Power Diagnostics

Egami, E. and Neugebauer, G. and Soifer, B. T. and Matthews, K. and Becklin, E. E. and Ressler, M. E. (2006) Subarcsecond Mid-Infrared Observations of NGC 6240: Limitations of Active Galactic Nucleus-Starburst Power Diagnostics. Astronomical Journal, 131 (3). pp. 1253-1261. ISSN 0004-6256. https://resolver.caltech.edu/CaltechAUTHORS:20170208-155142276

[img] PDF - Published Version
See Usage Policy.

787Kb
[img] PDF - Submitted Version
See Usage Policy.

618Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20170208-155142276

Abstract

In order to examine the relative importance of powerful starbursts and Compton-thick active galactic nuclei (AGNs) in NGC 6240, we have obtained mid-infrared images and low-resolution spectra of the galaxy with subarcsecond spatial resolution using the Keck telescopes. Despite the high spatial resolution (~200 pc) of our data, no signature of the hidden AGNs has been detected in the mid-infrared. The southern nucleus, which we show provides 80%–90% of the total 8–25 µm luminosity of the system, has a mid-infrared spectrum and a mid-/far-infrared spectral energy distribution consistent with starbursts. At the same time, however, it is also possible to attribute up to 60% of the bolometric luminosity to an AGN, consistent with X-ray observations, if the AGN is heavily obscured and emits mostly in the far-infrared. This ambiguity arises because the intrinsic variation of properties among a given galaxy population (e.g., starbursts) introduces at least a factor of a few uncertainty even into the most robust AGN-starburst diagnostics. We conclude that with present observations it is not possible to determine the dominant power source in galaxies when AGN and starburst luminosities are within a factor of a few of each other.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/499524DOIArticle
http://iopscience.iop.org/article/10.1086/499524/metaPublisherArticle
https://arxiv.org/abs/astro-ph/0511282arXivDiscussion Paper
Alternate Title:Sub-Arcsecond Mid-Infrared Observations of NGC 6240: Limitations of AGN-Starburst Power Diagnostics
Additional Information:© 2006 The American Astronomical Society. Received 2005 June 23; accepted 2005 November 3. We thank E. Sturm, A. S. Evans, and H. W. W. Spoon for providing us the ISO SWS spectra, the HST NICMOS images, and the ISOCAM CVF spectrum, respectively. We would also like to thank the anonymous referee for very helpful comments. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. This research has made use of the NASA/IPAC Extragalactic Database, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:galaxies: active — galaxies: individual (NGC 6240) — galaxies: interactions — galaxies: nuclei — galaxies: starburst — infrared: galaxies
Issue or Number:3
Record Number:CaltechAUTHORS:20170208-155142276
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170208-155142276
Official Citation:E. Egami et al 2006 AJ 131 1253
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74177
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:08 Feb 2017 23:57
Last Modified:03 Oct 2019 16:35

Repository Staff Only: item control page