Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-02T19:55:33.208Z Has data issue: false hasContentIssue false
  • English
  • Français

Multiband Photometry of NGC 7479 and NGC 7606

Published online by Cambridge University Press:  12 April 2016

A. M. Varela ,
J. A. L. Aguerri ,
M. Prieto  and
C. Muñoz-Tuñón
A. M. Varela
Affiliation:
Instituto de Astrofisica de Canarias, Tenerife, Spain
J. A. L. Aguerri
Affiliation:
Instituto de Astrofisica de Canarias, Tenerife, Spain
M. Prieto
Affiliation:
Department of Astronomy, University of Florida, Box 112055Gainesville, FLUSA
C. Muñoz-Tuñón
Affiliation:
Instituto de Astrofisica de Canarias, Tenerife, Spain

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present surface photometry in U BV RI passbands of the barred spiral galaxies NGC 7479 and NGC 7606, for which observations were obtained at the Cassegrain focus of the 2.5-m Isaac Newton Telescope at La Palma. Data are presented in the form of images and mean radial profiles from azimuthal fits of ellipses, giving the luminosity, ellipticities and position angles of the isophotes as functions of the galactocentric radii. Images in I-band are shown in Figure 1 of NGC 7479 (left) and NGC 7606 (right). These belong to a sample of galaxies with moderate circumnuclear starbursts. We are analyzing their structure to study the effects of departures from an axisymmetric potential for the dynamics of a galaxy. One objective of this study is to make a three-dimensional model of the bar and bulge using the method of photometric inversion. The sample consists of 27 spiral galaxies with and without a bar.

Type
Posters for Part I and Part II
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 123 - 125
Copyright
Copyright © Astronomical Society of the Pacific 1996