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The Morphology of the Spiral Galaxies: Encoded Information on the Origin and Evolution Mechanisms
Author(s) -
H. A. Harutyunian
Publication year - 2021
Publication title -
communications of the byurakan astrophysical observatory
Language(s) - English
Resource type - Journals
ISSN - 2579-2776
DOI - 10.52526/25792776-2021.68.1-50
Subject(s) - spiral (railway) , spiral galaxy , astrophysics , physics , dark matter , galaxy , elliptical galaxy , enhanced data rates for gsm evolution , lenticular galaxy , astronomy , artificial intelligence , computer science , mathematical analysis , mathematics
Consequences of the interaction between baryonic matter and dark energy carrier is considered for spinning objects. Some morphological features of spiral galaxies are used as fingerprints of formation processes to show that spiral arms of galaxies could be formed through mass ejection from the core of these objects. The Elmegreens’ arm classification allows one to find some opportune features for this end. For the same purpose, the ratio of vertical and radial sizes of some edge-on spiral galaxies found in deep fields and SDSS surveys is used.

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