Stellar velocity dispersion in ARP 220 and NGC 6240: Elliptical galaxies in formation

Details Stellar velocity dispersion in ARP 220 and NGC 6240: Elliptical galaxies in formation Stellar velocity dispersion in ARP 220 and NGC 6240: Elliptical galaxies in formation

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...437l..23d&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 437, no. 1, p. L23-L26

Astronomy and Astrophysics

Astronomy

62

Elliptical Galaxies, Galactic Evolution, Interacting Galaxies, Velocity Distribution, Absorption Spectra, Brightness Distribution, Infrared Astronomy, Light Curve

Scientific paper

We present high-resolution (R is approximately 7000) spectra of the 2.3 micron CO absorption bandhead of two luminous merging galaxies, NGC 6240 and Arp 220, obtained with CGS4 on the United Kingdom Infrared Telescope. We have also secured subarcsecond images of NGC 6240 at 2.2 micron using the Montreal Infrared Camera (MONICA) on the Canada-France-Hawaii Telescope (CFHT). The velocity dispersion (sigmaobs = FWHM/2.354) inferred from the broadening of the CO bandhead in the central 2 sec of the brightest nucleus of NGC 6240 is 359 +/- 21 km/s, which is among the highest values ever found in the center of a galaxy. Arp 220 shows a velocity dispersion of 150 +/- 21 km/s. The infrared light profile of NGC 6240 beyond a radius of 0.7 sec is well fitted by an r1/4 law, but the overall brightness distribution is best represented by a shallower profile such as a King (1966) profile with a core radius of 0.20 kpc. Both Arp 220 and NGC 6240 have mass densities, velocity dispersions, and central surface brightnesses consistent with the fundamental parameter plane of elliptical galaxies.

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