CaltechAUTHORS
  A Caltech Library Service

The near-infrared morphology of ultraluminous infrared galaxies

Carico, David P. and Graham, James R. and Matthews, K. and Wilson, T. D. and Soifer, B. T. and Neugebauer, G. and Sanders, D. B. (1990) The near-infrared morphology of ultraluminous infrared galaxies. Astrophysical Journal, 349 (1). L39-L42. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20170301-135109996

[img] PDF - Published Version
See Usage Policy.

553Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20170301-135109996

Abstract

Near-infrared images at 1.25 μm, 1.65 μm, and 2.2 μm have been obtained of nine galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR) ≥ 10^(12) L_☉. Two of the 2.2 μm images reveal previously undetected double nuclei, increasing the number of close double nuclei known for this sample from two to four. For three of these four sources, the colors of both nuclei are substantially different from those of normal spiral galaxies, indicating that the high activity state in high-luminosity mergers tends to occur in both nuclei. Three sources show 2.2 μm emission that is more centrally concentrated than the emission at 1.3 μm, a result that can be explained as the effects of dust emission and/or extinction or, alternatively, as the result of direct emission at 2.2 μm from the accretion disk of a central active galactic nucleus. Implications of these results for the model that galaxy collisions lead to quasar formation are briefly discussed. Finally, from the frequency and separation of the double nucleus sources, the lifetime of the ultraluminous phase of galaxies is estimated to be ~ 4 x 10^8 yr.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/185646DOIArticle
http://adsabs.harvard.edu/abs/1990ApJ...349L..39CADSArticle
Additional Information:© 1990 American Astronomical Society. Received 1989 September 6; accepted 1989 November 16. We thank the night assistants at the Hale telescope, J. Carasco and S. Staples, and the entire staff at Palomar Observatory. S. Lin made substantial contributions to the construction of the near-infrared camera, and V. Heron wrote most of the data acquisition software for the camera. Discussions with S. Phinney and W. Sargent were most helpful, as were the suggestions provided by the referee, G. Wynn-Williams. Ground-based infrared astronomy at Caltech is supported by a grant from the NSF.
Funders:
Funding AgencyGrant Number
NSFUNSPECIFIED
Subject Keywords:galaxies: interactions galaxies: nuclei infrared: general quasars
Record Number:CaltechAUTHORS:20170301-135109996
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170301-135109996
Official Citation:The near-infrared morphology of ultraluminous infrared galaxies Carico, D. P., Graham, J. R., Matthews, K., Wilson, T. D., Soifer, B. T., Neugebauer, G. Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 349, Feb. 1, 1990, p. L39-L42
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:74653
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:02 Mar 2017 03:42
Last Modified:02 Mar 2017 03:42

Repository Staff Only: item control page