Environment Dependence of Disk Morphology of Spiral Galaxies
H. B. Ann

TL;DR
This study investigates how the morphology of spiral galaxy disks, including arm class, Hubble type, and bar type, depends on environmental factors like local density, projected distance, and tidal index, revealing strong correlations especially for arm class and Hubble type.
Contribution
It provides a detailed analysis of the environmental influences on various disk morphology features of spiral galaxies, highlighting the differing impacts of local density and nearest neighbor proximity.
Findings
Arm class and Hubble type strongly depend on environment.
Grand design and early-type fractions increase with environmental measures.
Bar type shows weak dependence, mainly on projected distance.
Abstract
We analyze the dependence of disk morphology (arm class, Hubble type, bar type) of nearby spiral galaxies on the galaxy environment by using local background density (), projected distance (), and tidal index () as measures of the environment. There is a strong dependence of arm class and Hubble type on the galaxy environment, while the bar type exhibits a weak dependence with a high frequency of SB galaxies in high density regions. Grand design fractions and early-type fractions increase with increasing , , and , while fractions of flocculent spirals and late-type spirals decrease. Multiple-arm and intermediate-type spirals exhibit nearly constant fractions with weak trends similar to grand design and early-type spirals. While bar types show only a marginal dependence on , they show a fairly clear dependence on with a…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Remote Sensing in Agriculture
