Volume 421, Number 2, July II 2004
|Page(s)||595 - 601|
|Published online||22 June 2004|
Deprojecting spiral galaxies using Fourier analysis. Application to the Ohio sample *
DEIM, Campus Sescelades, Avd. dels Països Catalans 26, 43007 Tarragona, Spain
2 Observatoire de Marseille, 2 place Le Verrier, 13248 Marseille Cedex 04, France
3 School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD, UK
Corresponding author: C. García-Gómez, firstname.lastname@example.org
Accepted: 7 April 2004
We use two new methods developed recently (Barberà et al. [CITE], A&A, 415, 849), as well as information obtained from the literature, to calculate the orientation parameters of the spiral galaxies in the Ohio State University Bright Galaxy Survey. We compare the results of these methods with data from the literature, and find in general good agreement. We provide a homogeneous set of mean orientation parameters which can be used to approximately deproject the disks of the galaxies and facilitate a number of statistical studies of galaxy properties.
Key words: galaxies: structure / galaxies: spiral
© ESO, 2004
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