EDP Sciences
Free Access
Volume 409, Number 3, October III 2003
Page(s) 867 - 878
Section Galactic structure and dynamics
DOI https://doi.org/10.1051/0004-6361:20031165
Published online 17 November 2003

A&A 409, 867-878 (2003)
DOI: 10.1051/0004-6361:20031165

ISO spectroscopy of star formation and active nuclei in the luminous infrared galaxy NGC 6240

D. Lutz1, E. Sturm1, R. Genzel1, H. W. W. Spoon2, A. F. M. Moorwood3, H. Netzer4 and A. Sternberg4

1  Max-Planck-Institut für extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany
    e-mail: lutz@mpe.mpg.de;sturm@mpe.mpg.de;genzel@mpe.mpg.de
2  Kapteyn Institute, PO Box 800, 9700 AV Groningen, The Netherlands
    e-mail: spoon@astro.rug.nl
3  European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany
    e-mail: amoor@eso.org
4  School of Physics and Astronomy and Wise Observatory, Raymond and Beverly Sackler Faculty of Exact Sciences, Tel Aviv University, Ramat Aviv, Tel Aviv 69978, Israel
    e-mail: netzer@wise1.tau.ac.il;amiel@wise1.tau.ac.il

(Received 23 April 2003 / Accepted 22 July 2003)

We present Infrared Space Observatory mid- and far-infrared spectroscopy of the merging galaxy NGC 6240 , an object presenting many aspects of importance for the role of star formation and AGN activity in [ultra]luminous infrared galaxies. The mid-infrared spectrum shows starburst indicators in the form of low excitation fine-structure line emission and aromatic "PAH" features. A strong high excitation [O IV] line is observed which most likely originates in the Narrow Line Region of an optically obscured AGN. NGC 6240 shows extremely powerful emission in the pure rotational lines of molecular hydrogen. We argue that this emission is mainly due to shocks in its turbulent central gas component and its starburst superwind. The total shock cooling in infrared emission lines accounts for ~0.6% of the bolometric luminosity, mainly through rotational H 2 emission and the [O I] 63 $~\mu$m line. We analyse several ways of estimating the luminosities of the starburst and the AGN in NGC 6240 and suggest that the contributions to its bolometric luminosity are most likely in the range 50-75% starburst and 25-50% AGN.

Key words: galaxies: individual: NGC 6240 -- infrared: galaxies -- galaxies: active -- galaxies: starburst

Offprint request: D. Lutz, lutz@mpe.mpg.de

SIMBAD Objects

© ESO 2003

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.