Deprojecting spiral galaxies using Fourier analysis. Application to the Ohio sample

Details Deprojecting spiral galaxies using Fourier analysis. Application to the Ohio sample Deprojecting spiral galaxies using Fourier analysis. Application to the Ohio sample

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...421..595g&link_type=abstract

Astronomy and Astrophysics, v.421, p.595-601 (2004)

Astronomy and Astrophysics

Astrophysics

6

Galaxies: Structure, Galaxies: Spiral

Scientific paper

We use two new methods developed recently (Barberàet al. \cite{bar03}, 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.
Table 1 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/421/595

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