NGC 6240: merger-induced star formation and gas dynamics^⋆

¹ Max Planck Institut für extraterrestrische Physik, Postfach 1312, 85741 Garching, Germany
e-mail: hauke@mpe.mpg.de
² Universitätssternwarte, Scheinerstrasse 1, 81679 München, Germany
³ Center for Adaptive Optics, University of California, Santa Cruz, CA 95064, USA
⁴ Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands

Received: 5 July 2010
Accepted: 26 August 2010

Abstract

We present spatially resolved integral field spectroscopic K-band data at a resolution of 0.13″ (60 pc) and interferometric CO(2–1) line observations of the prototypical merging system NGC 6240. Despite the clear rotational signature, the stellar kinematics in the two nuclei are dominated by dispersion. We use Jeans modelling to derive the masses and the mass-to-light ratios of the nuclei. Combining the luminosities with the spatially resolved Brγ equivalent width shows that only 1/3 of the K-band continuum from the nuclei is associated with the most recent star forming episode; and that less than 30% of the system’s bolometric luminosity and only 9% of its stellar mass is due to this starburst. The star formation properties, calculated from typical merger star formation histories, demonstrate the impact of different assumptions about the star formation history. The properties of the nuclei, and the existence of a prominent old stellar population, indicate that the nuclei are remnants of the progenitor galaxies’ bulges.