Fractal Dimension of Galaxy Isophotes

In this paper we investigate the use of the fractal dimension of galaxy isophotes in galaxy classification. We have applied two different methods for determining fractal dimensions to the isophotes of elliptical and spiral galaxies derived from CCD images. We conclude that fractal dimension alone is...

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Bibliographic Details
Published inThe Astronomical journal Vol. 138; no. 3; pp. 941 - 950
Main Authors Thanki, Sandip, Rhee, George, Lepp, Stephen
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.09.2009
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ISSN1538-3881
0004-6256
1538-3881
DOI10.1088/0004-6256/138/3/941

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Summary:In this paper we investigate the use of the fractal dimension of galaxy isophotes in galaxy classification. We have applied two different methods for determining fractal dimensions to the isophotes of elliptical and spiral galaxies derived from CCD images. We conclude that fractal dimension alone is not a reliable tool but that combined with other parameters in a neural net algorithm the fractal dimension could be of use. In particular, we have used three parameters to segregate the ellipticals and lenticulars from the spiral galaxies in our sample. These three parameters are the correlation fractal dimension D corr, the difference between the correlation fractal dimension and the capacity fractal dimension D corr - D cap, and, thirdly, the B - V color of the galaxy.
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ISSN:1538-3881
0004-6256
1538-3881
DOI:10.1088/0004-6256/138/3/941