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A Multiwavelength Study of the Barred Spiral Galaxy NGC 7479

Published online by Cambridge University Press:  12 April 2016

S. Laine  and
S. T. Gottesman
S. Laine
Affiliation:
University of Florida, Astronomy Department, P.O. Box 112055 Gainesville, FL 32611-2055, U.S.A.
S. T. Gottesman
Affiliation:
University of Florida, Astronomy Department, P.O. Box 112055 Gainesville, FL 32611-2055, U.S.A.

Abstract

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The detailed investigation of the activity and dynamics in NGC 7479 confirms the importance of understanding individual galaxies. We have discovered an S-shaped emission structure in 21 cm continuum. This detection together with strong nuclear 10 μm and Hα emission may imply the existence of a central massive black hole. We also address the origin of the asymmetric spiral structure in NGC 7479. The lack of any visible companion and the unperturbed H I velocity field suggest that the asymmetry has an internal origin.

Type
Posters of Part VII and Part VIII
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 495 - 497
Copyright
Copyright © Astronomical Society of the Pacific 1996