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Morphology and Structures of Nearby Dwarf Galaxies

Published online by Cambridge University Press:  09 May 2016

Mira Seo  and
H. B. Ann
Mira Seo
Affiliation:
Dept. of Earth Science, Pusan National University 609-735, Busan, Korea email: mrseo@pusan.ac.kr, hbann@pusan.ac.kr
H. B. Ann
Affiliation:
Dept. of Earth Science, Pusan National University 609-735, Busan, Korea email: mrseo@pusan.ac.kr, hbann@pusan.ac.kr
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Abstract

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We applied GALFIT and STARLIGHT to the r-band images and spectra, respectively, of ~1,100 dwarf galaxies to analyze the structural properties and stellar populations. In most cases, single component with n = 1 ~ 1.5 well describes the luminosity distribution of dwarf galaxies. However, a large fraction of dS0, dEbc, and dEblue galaxies show sub-structures such as spiral arms and rings. There is a bimodal distributions of stellar ages in dS0 galaxies. But other sub-types of dwarf galaxies show a single peak in the stellar distributions.

Keywords

galaxiesdwarfstructurepopulation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Issue S317: The General Assembly of Galaxy Halos: Structure, Origin and Evolution , August 2015 , pp. 348 - 349
Copyright
Copyright © International Astronomical Union 2016 

References

Ann, , Seo, , Ha, 2015, ApJS, 217, 27Google Scholar
Cid Fernandes, R., Mateus, A., Sodre, L., Stasinska, G., & Gomes, J. M. 2005, MNRAS, 358, 363Google Scholar
Peng, C. Y., Ho, L. C., Impey, C. D., & Rix, H.-W. 2002, AJ, 124, 266Google Scholar
Peng, C. Y., Ho, L. C., Impey, C. D., & Rix, H.-W. 2010, AJ, 139, 2097Google Scholar