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3.11. Resolved structure in the nuclear region of the ultraluminous infrared galaxy Mrk 273

Published online by Cambridge University Press:  25 May 2016

J.H. Knapen ,
S. Laine ,
J.A. Yates ,
A. Robinson ,
A.M.S. Richards ,
R. Doyon  and
D. Nadeau
J.H. Knapen
Affiliation:
Department of Physical Sciences, University of Hertfordshire, Hatfield, Herts AL10 9AB, UK
S. Laine
Affiliation:
Department of Physical Sciences, University of Hertfordshire, Hatfield, Herts AL10 9AB, UK
J.A. Yates
Affiliation:
Department of Physical Sciences, University of Hertfordshire, Hatfield, Herts AL10 9AB, UK
A. Robinson
Affiliation:
Department of Physical Sciences, University of Hertfordshire, Hatfield, Herts AL10 9AB, UK
A.M.S. Richards
Affiliation:
Nuffield Radio Astronomy Laboratories, University of Manchester, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, UK
R. Doyon
Affiliation:
Observatoire du Mont Mégantic and Département de Physique, Université de Montréal, C.P. 6128, Succursale Centre Ville, Montréal (Québec), H3C 3J7 Canada
D. Nadeau
Affiliation:
Observatoire du Mont Mégantic and Département de Physique, Université de Montréal, C.P. 6128, Succursale Centre Ville, Montréal (Québec), H3C 3J7 Canada

Extract

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As an example of the power of near-infrared (NIR) Adaptive Optics imaging in the detailed study of central regions of galaxies, we present high-resolution K-band imaging of Mrk 273, in combination with interferometric radio continuum data.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 111 - 112
Copyright
Copyright © Kluwer 1998 

References

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Knapen, J. H., Laine, S., Yates, J., Robinson, A., Richards, A.M.S., Doyon, R., Nadeau, D. 1997, ApJL, in press.Google Scholar
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