Hostname: page-component-76fb5796d-5g6vh Total loading time: 0 Render date: 2024-04-26T23:47:34.411Z Has data issue: false hasContentIssue false
  • English
  • Français

Structural Components of NGC 5850

Published online by Cambridge University Press:  12 April 2016

M. Prieto ,
J. A. López ,
A. M. Varela ,
C. Muñoz-Tuñón  and
S. Gottesman
M. Prieto
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain 38200
J. A. López
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain 38200
A. M. Varela
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain 38200
C. Muñoz-Tuñón
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Spain 38200
S. Gottesman
Affiliation:
Department of Astronomy, University of Florida, Gainesville, FL 112055

Abstract

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.

Here we present a study of the structural components of the barred galaxy NGC 5850 using U, B and I photometry. After subtracting a bulge+disk model from the observed image, we obtain the bar and other non-axisymmetric structures. We determine the position of the ILR from the ellipticity and position angle profiles of the isophotes.

Type
Posters of Part VII and Part VIII
Information
International Astronomical Union Colloquium , Volume 157: Barred Galaxies , 1996 , pp. 480 - 482
Copyright
Copyright © Astronomical Society of the Pacific 1996