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Published byBaldric McCarthy Modified over 9 years ago
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Satellite Systems In The Local Universe 안홍배 Morphology and Environment of Nearby Galaxies 안홍배 ARCSEC Workshop 22-23, Jan 2006 SDSS KSG Hiwon, 2008
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Galaxy Zoo
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Dwarfs: dE, N dE dEpec dEblue
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Blue dwarf ellipticals
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Morphology and Luminosity of dwarfs
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Colors and magnitudes of dwarfs
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Density distribution
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CAS
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CAS plus
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Sersic index
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Concluding Remarks Morphology is an integral property of a galaxy that reflects its formation and evolution process as well as its dynamical structures. The local background density is a critical parameter that controls the galaxy morphology. There is no difference between the dwarf irregulars and blue dwarf ellipticals except for the apparent roundness. Thus, apparent shape does not play decisive roles in defining galaxy morphology.
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In case of satellite galaxies Ann, Park & Choi (2008)
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Need more versatile classifier to differentiate barred galaxies from non- barred ones and lenticulars from ellipticals.
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Blue dwarf ellipticals
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