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The Circumnuclear Spiral Pattern of NGC 5427

Published online by Cambridge University Press:  03 June 2010

J. A. Hernandez-Jimenez ,
H. Dottori ,
P. Grosbøl  and
N. Vera-Villamizar
J. A. Hernandez-Jimenez
Affiliation:
Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Av. Bento Gonçalves 9500, 91501-970 Porto Alegre, RS, Brazil Email: [email protected]
H. Dottori
Affiliation:
Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Av. Bento Gonçalves 9500, 91501-970 Porto Alegre, RS, Brazil Email: [email protected]
P. Grosbøl
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, DE 85748 Garching, Germany
N. Vera-Villamizar
Affiliation:
Escuela de Física, Univeridad Pedagogica y Tecnologica de Colombia, Av. Central del Norte, Tunja, Colombia
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We have studied Hubble Space Telescope archive imagery of the central region of the Seyfert 2 galaxy NGC 5427. The images were taken with F606W (V-band) and F160W (H-band) filters with the Wide Field and Planetary Camera 2 and the Near Infrared Camera and Multi-Object Spectrometer, respectively.

Keywords

methods: numericaltechniques: photometricgalaxies: bulgesgalaxies: individual (NGC 5427)galaxies: nucleigalaxies: Seyfertgalaxies: spiralgalaxies: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S267: Co-Evolution of Central Black Holes and Galaxies , August 2009 , pp. 331
Copyright
Copyright © International Astronomical Union 2010

References

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