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Galaxies
After individual compact objects and sun-like stars, galaxies are the next larger structured objects that are presented here. We start with our... -
Fundamental Plane of Groups and Clusters of Galaxies: Distances and Pecular Velocities of Superclusters of Galaxies on Small Scales
AbstractThis work is a continuation of the work of Kopylova and Kopylov published in 2016 on constructing the fundamental plane (FP) of groups and...
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Galaxies
Various classification schemes for galaxies are introduced, including the Hubble-de Vaucouleurs sequence, as well as other classes of galaxy:... -
Galaxies and Clusters of Galaxies in Observations and Numerical Models
AbstractAn analysis of the properties of 1157 galaxies, groups and clusters of galaxies confirms the dependence of the virial velocity on the halo...
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Satellites around Edge-on Galaxies. I. Dynamical Masses
AbstractWe have undertaken a search for satellites around edge-on galaxies in the EGIPS catalog, which contains 16 551 objects with declinations...
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Evolutionary paths of active galactic nuclei and their host galaxies
The tight correlations between the masses of supermassive black holes (BHs) and the properties of their host galaxies suggest that BHs co-evolve with...
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Dilution of chemical enrichment in galaxies 600 Myr after the Big Bang
The evolution of galaxies throughout the last 12 Gyr of cosmic time has followed a single, universal relation that connects star-formation rates...
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Surface Photometry of 50 Dwarf Galaxies in the Local Volume
Results of surface photometry of 50 galaxies in the Local Volume based on archived images obtained with the Hubble Space Telescope are presented....
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A Search for New Dwarf Galaxies Outside the Nearby Groups
We undertook a search for new nearby dwarf galaxies outside the known groups in the Local Volume using the data on DESI Legacy Imaging Surveys. In a...
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The Evolution of Evolved Galaxies
The plethora of high redshift multifrequency surveys currently under way, that were extensively illustrated at this meeting will shortly provide us... -
Rotational curves decomposition of spiral galaxies using least square non-linear regression
Dark Matter mass distribution is studied in a Cold Dark Matter Universe using Navarro–Frenk–White density profile for Dark Matter (DM) in spiral...
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Distances to 24 Dwarf Galaxies
AbsrtactStellar photometry of 24 dwarf galaxies was carried out using the archival images of the Hubble Space Telescope. The resulting...
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Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ΛCDM prediction
Galaxies of different types are not equally distributed in the Local Universe. In particular, the supergalactic plane is prominent among the...
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Radio Properties of the Low-Redshift Isolated Galaxies with Active Nuclei
AbstractThe properties of 61 isolated galaxies with active nuclei (isolated AGNs) in the radio frequency range at redshifts z < 0.05 have been...
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Distances to 10 Nearby Galaxies Observed with the Hubble Space Telescope
Images of 10 galaxies in F814W and F606W filters obtained on the Hubble Space Telescope (HST) are used to construct color-magnitude diagrams for the...
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Possibilities of identifying members from Milky Way satellite galaxies using unsupervised machine learning algorithms
A detailed study of stellar populations in Milky Way (MW) satellite galaxies remains an observational challenge due to their faintness and fewer...
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Spectroscopic confirmation of four metal-poor galaxies at z = 10.3–13.2
Finding and characterizing the first galaxies that illuminated the early universe at cosmic dawn is pivotal to understand the physical conditions and...
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Fact: Many SCUBA Galaxies Harbour AGNs
Deep SCUBA surveys have uncovered a large population of ultra-luminous galaxies at z>1. These sources are often assumed to be starburst galaxies, but...