Galaxy Morphological Classification with Zernike Moments and Machine Learning Approaches
Classifying galaxies is an essential step for studying their structures and dynamics. Using GalaxyZoo2 (GZ2) fractions thresholds, we collect 545 and 11,735 samples in nongalaxy and galaxy classes, respectively.
Hamed Ghaderi +2 more
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THE CARNEGIE-IRVINE GALAXY SURVEY. III. THE THREE-COMPONENT STRUCTURE OF NEARBY ELLIPTICAL GALAXIES
Motivated by recent developments in our understanding of the formation and evolution of massive galaxies, we explore the detailed photometric structure of a representative sample of 94 bright, nearby elliptical galaxies, using high-quality optical images
Huang, Song +4 more
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Near IR imaging of Centaurus group dwarf elliptical galaxies
Detailed studies of dwarf galaxies in the Local Group have revealed an amazing diversity in their star formation histories. Young and intermediate-age stellar populations are observed in some gas-poor dwarf ellipticals, like Fornax and Carina, where ...
Zoccali, M +4 more
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JWST NIRCam Observations of the Globular Cluster Population of RXJ 2129.7+0005
We present an analysis of the globular cluster (GC) population in the galaxy cluster RXJ 2129.7+0005 ( z = 0.234) based on JWST NIRCam imaging in three filters: F115W, F150W, and F200W.
Kaitlyn E. Keatley, William E. Harris
doaj +1 more source
Unequal-mass galaxy merger remnants: spiral-like morphology but elliptical-like kinematics [PDF]
4 pages, 3 figuresIt is generally believed that major galaxy mergers with mass ratios in the range 1:1-3:1 result in remnants that have properties similar to elliptical galaxies, and minor mergers below 10:1 result in disturbed spiral galaxies.
F. Combes +9 more
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Modeling the Ages and Chemical Abundances of Elliptical Galaxies
Spectroscopic studies of elliptical galaxies show that their stellar population ages, mean metallicity, and α enhancement traced by [Mg/Fe] all increase with galaxy stellar mass or velocity dispersion.
Nicole Marcelina Gountanis +5 more
doaj +1 more source
Scaling Relations of Early-Type Galaxies in MOND
We investigate the shape and morphology of early-type galaxies (ETGs) within the framework of Modified Newtonian Dynamics (MOND). Building on our previous studies, which demonstrated that the monolithic collapse of primordial gas clouds in MOND produces ...
Robin Eappen, Pavel Kroupa
doaj +1 more source
Energy Evolution in the Progenitor of Galaxy Shells: A Semi-analytical Model
The stellar shells surrounding an elliptical galaxy, as remnants of a dwarf galaxy disrupted during merging, reveal the distribution of energy and angular momentum of the progenitor dwarf galaxy. We develop a semi-analytical model to describe the changes
Beibei Guo +3 more
doaj +1 more source
Automatic Detection of Galaxy Type From Datasets of Galaxies Image Based on Image Retrieval Approach
This paper presents a new approach for the automatic detection of galaxy morphology from datasets based on an image-retrieval approach. Currently, there are several classification methods proposed to detect galaxy types within an image.
Mohamed Abd El Aziz +2 more
doaj +1 more source
The Distribution of Elliptical Galaxy Shapes
: An estimate of the parent distribution function of the intrinsic shapes of elliptical galaxies is calculated by fitting photometric and kinematic data from the Davies and Birkinshaw sample to a set of dynamical models. 1.
Stromlo Symposium +5 more
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