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Dark matter effect on the weak deflection angle by black holes at the center of Milky Way and M87 galaxies
In this paper, we investigated the effect of dark matter on the weak deflection angle by black holes at the galactic center. We consider three known...
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Simulations of galaxies in an expanding Universe with modified Newtonian dynamics (MOND) and with modified gravitational attractions (MOGA)
The stability of galaxies is either explained by the existence of dark matter or caused by a modification of Newtonian acceleration (MOND). Here, we...
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Dark Matter in the Center of LSB and Dwarf Galaxies from H $\alpha$ Observations
This work is focused on the preliminary results of the observations of H... -
The Tully-Fisher Relation for Compact Group Galaxies
Compact groups of galaxies are systems with high densities and low velocity dispersions, where galaxy interactions should play a major role in the... -
The Effect of Gaseous Dissipation on the Fate of Supermassive Black Holes in Merging Galaxies
We analyze the effect of dissipation on the orbital evolution of supermassive black holes (SMBHs) using high-resolution gasdynamical simulations of... -
Cosmological Distance Scale. Part 14: “Hubble Bubble” and the Gravitational Dipole
Drawing on astronomical discoveries made in the past 25 years, the paper discusses possible causes of the phenomenon perceived as the “accelerated...
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From the Earliest Seeds to Today’s Supermassive Black Holes
I review scenarios for the assembly of supermassive black holes (MBHs) at the center of galaxies that trace their hierarchical build-up far up in the... -
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Enhanced \(m = 1\) WKB instabilities in nearly Keplerian stellar discs due to the presence of gas
Dynamical evolution of galaxies is a complex process, especially the centers. Gravitationally coupled gas and stellar discs have been observed to...
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Galaxy Cluster A 2142: Halo Boundary, “Red Sequence”, Properties of Galaxies Based on SDSS
Abstract —Here we present results of studying the dynamics of galaxies, properties of early-type galaxies, properties of galaxies with the quenched...
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Presence of Dual Structure in Galaxy Clusters from CfA2 Redshift Survey which Reveals High-Energy \({\gamma}\)-Associations on Fermi/LAT 12-Year Point Source Catalog 4FGL DR3
AbstractThe presence of dual structure in 13 clusters of galaxies from CfA2 Redshift Survey is discussed. The spatial distributions of galaxies and...
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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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Formation of the First Supermassive Black Holes
Understanding the emergence of the first supermassive black holes, and hence the first quasars, is a crucial ingredient for models of reionization... -
The Scalar Field Dark Matter Model: A Braneworld Connection
This work is a review for the progress of the scalar field dark matter (SFDM) hypothesis. Here we outline a possible brane world model justifying the... -
Chemo-Photometric Models of Ring Galaxies
The peculiar ring galaxies are formed as a result of cosmic interaction. An intruder galaxy plunges through the center of a disk galaxy triggering... -
Radiative Feedback from Quasars and the Growth of Supermassive Black Holes
We discuss the role of feedback via photoionization and Compton heating in the co-evolution of massive black holes at the center of spheroidal... -
Molecular and Atomic Gas in Star-forming Complexes: NGC 5194, NGC 5457, NGC 628, and NGC 6946
Abstract —We use observations of CO and HI emission in star-forming complexes (SFCs) in galaxies NGC 5457, NGC 5194, NGC 628, and NGC 6946 to search...
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The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way
Galactic outflows are ubiquitous in galaxies containing active star formation or supermassive black hole activity. The presence of a large-scale...
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Evidence for Massive Black Holes in the Nuclei of Active Galaxies from Gamma-Ray Observations
According to our present knowledge, Active Galactic Nuclei (AGNs) consist of massive black holes which accrete matter from their environments. By...