Astrophysics

Papers
(The TQCC of Astrophysics is 2. The table below lists those papers that are above that threshold based on CrossRef citation counts [max. 250 papers]. The publications cover those that have been published in the past four years, i.e., from 2021-03-01 to 2025-03-01.)
ArticleCitations
On the Problem of the Galaxy Alignment with Groups and Clusters12
On the Extended Blazar Sequence for γ-Ray Emitting Active Galactic Nuclei12
Quantitative Analysis of the Spectra of CQ Tau and UX Ori Stars Outside Eclipses According to the Nordic Optical Telescope Data10
Time Dependent Radiative Transfer Problems in a One-Dimensional Medium8
Features of the Magnetic Field Behavior of the Ae/Be Star HD1900737
On the Centenary of L. V. Mirzoyan6
Theory of Classical Gaseous Polytropes in an Integral Representation. I. Some General Results5
TYC 1417-891-1 and TYC 1478-742-1: Eclipsing Variable Stars. The Gaia EDR3 and TESS Photometric Data5
Properties of Hot Quark Matter with Neutrino Confinement in the NJL Model5
Photometric Study and Orbital Solution for Some Newly Discovered Eclipsing Binary Systems5
Higher-Dimensional Anisotropic Modified Holographic Ricci Dark Energy Cosmological Model in Lyra Manifold5
Oxygen-Rich Cool Stars in the Cepheus Region. New Spectroscopic Observations of Selected Objects from the KP2001 Catalog4
KIC 7732964 – A Possible Candidate FK Com-Type Star4
Viscous Ricci Dark Energy Cosmological Models in Brans-Dicke Theory4
Problems with Root-Mean-Square Values of the Magnetic Field of Ap Stars. I.4
Motion of a Particle in the Field of an Infinite Flat Slab3
Viscous Plane Symmetric String Cosmological Model in f (R) Gravity3
Electromagnetic Properties of Stellar Matter. I. Dielectric Permeability of a Hot Rarefied Plasma with Abundant Production of Electron-Positron Pairs3
Solutions for Massless Bosons in the Mannheim-Kazanas Space-Time3
Photometric Study and Evolutionary State for Some Newly Discovered W UMA Systems3
Magnetic Field Structures of Chemically Peculiar Stars. II. HD98088, HD182180, HD221218, HD3181073
Compton Scattering in Plane Media: Polarization of Radiation and Azimuthal Independence. II. Results of Calculations3
Fermionic Vacuum Stresses in Models with Toroidal Compact Dimensions3
Photometric Study of the Asynchronous Polar IGR J19552+0044 in 2019-20223
Escape Probability and Mean Numbers of Photon Scatterings. I. Exact and Asymptotic Formulas2
Several Star-Formation Regions in the Southern Hemisphere2
Renyi Holographic Dark Energy and Its Behaviour in f(G) Gravity2
Classification of BLL Blazars by Optical Activity Types2
Optical Classification of BZG Objects from the BZCAT Blazar Catalog2
Multilayer Spherical Stellar Clusters with Uniform Density2
The Mysterious Radcliffe Wave2
Catalog of X-Ray Active Galactic Nuclei Based on ROSAT BSC and FSC Sources2
On a Possible Mechanism for the Start or Resumption of Activity of Radio Galaxies in Clusters of Galaxies2
Correction to: Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation2
Physical Acceptability of the Renyi Holographic Dark Energy Model Under the Hubble's Cutoff in f (T, B) Gravity2
Distances to 10 Nearby Galaxies Observed with the Hubble Space Telescope2
Isospin-Asymmetric Cold Nuclear Matter in the Relativistic Mean-Field Theory with a Scalar-Isovector Interaction Channel2
Fermionic Condensate in de Sitter Spacetime2
WASP-18b Secondary Eclipses Revisited Using TESS Observation2
Modified Tsallis Holographic Dark Energy2
Variation of Doppler Velocities and D3 Spicule Half-Widths2
Hot Quark Matter with Neutrino Confinement in Terms of the Local Nambu - Jona-Lasinio SU(3) Model2
BSN: First Photometric Light Curve Analysis of Two W-Type Contact Binary Systems OP Boo and V0511 Cam2
Induced Electromagnetic Radiation from a Charged Cloud in a Plane Gravitational Wave2
Halo Effect on Bar Rotation in Galaxies2
Modified Renyi Holographic Dark Energy (MRHDE) in f(R, T) Theory of Gravity2
Circumstellar Properties of the Herbig Be Star HD 259431. I. Signatures of Magnetospheric Accretion2
Discrepancy between Values of the Hubble Constant Obtained by Different Methods2
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