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3D-structure of galactic disks

Published online by Cambridge University Press:  09 February 2015

Ekaterina Chudakova
Ekaterina Chudakova*
Affiliation:
Sternberg Astronomical Institute, Lomonosov Moscow State University, email: [email protected]
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Abstract

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We suggest a new photometric method to estimate thicknesses of galactic disks which is working for the galaxies seen under arbitrary inclination. We have applied our method to 45 galaxies from the open SDSS archive and to 57 galaxies from the Spitzer Survey S4G).

Keywords

galaxies: elliptical and lenticularcD - galaxies: spiral - galaxies: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 306
Copyright
Copyright © International Astronomical Union 2015 

References

Erwin, P., Pohlen, M., & Beckman, J. E. 2008, AJ, 135, 20CrossRefGoogle Scholar
Gutiérrez, L., Erwin, P., Aladro, R., & Beckman, J. E. 2011, AJ, 142, 145CrossRefGoogle Scholar
Muñoz-Mateos, J. C., Sheth, K., Gil de Paz, A., et al. 2013, ApJ, 771, aid 59CrossRefGoogle Scholar
Chudakova, E. M. & Sil'chenko, O. K., 2014, Astron. Rep., 58, 281CrossRefGoogle Scholar