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 2022-08-01 to 2026-08-01.)
ArticleCitations
Optical Classification of BZG Objects from the BZCAT Blazar Catalog43
Correction to: Accelerating Kaluza-Klein Universe in Modified Theory of Gravitation16
Induced Electromagnetic Radiation from a Charged Cloud in a Plane Gravitational Wave11
A Study on Geodesics and Lifespan of the Rindler-Modified Schwarzschild Black Hole. I. Time-Like Geodesics8
Study of Periodic Cosmic Evolution in Modified f(Q, T) Gravity Theory8
A Study on Geodesics and Lifespan of the Rindler-Modified Schwarzschild Black Hole. II. Null Geodesics and Black Hole Lifespan8
Methanimine in Cool Cosmic Objects Using Accurate Collisional Rate Coefficients8
Magnetic Field Structures of Chemically Peculiar Stars. II. HD98088, HD182180, HD221218, HD3181078
Classification of BLL Blazars by Optical Activity Types6
Doppler Velocity and Spectral Line Width Variations in Solar Spicules and Prominences6
Thermodynamics and its Quantum Correction of Vacuum Nonsingular Black Hole6
Activity of the Star TOI-6255 and Atmospheric Mass Loss from its Planet5
On the Origin of Emission in the White-Light Continuum in Powerful Stellar and Solar Flares5
Starspot Activity of Moving Groups from Tess Mission Archive Data5
Activity of Stars with Planets in the Habitable Zone5
Activity Cycles of dM4e Dwarf GJ 12435
Topological Casimir Effect in Models with Helical Compact Dimensions4
Transverse Gradients of Longitudinal Magnetic Field in Active Regions with Different Levels of Flare Productivity. II. Statistical Analysis4
Swampland Criteria and Neutrino Generation in a Non-Cold Dark Matter Universe4
Atmospheric Mass Loss of Planet WASP-195b4
Uniform models of neutron and quark (strange) stars in general relativity3
Thermodiffusion Unipolar Electric Generator3
Activity of the Star Gl 414A with Two Planets and its Effect on the Loss of Mass of the Atmosphere of the Planet Gl 414A b3
Spectral Variations and Physical Conditions of BY Draconis in the Ultraviolet3
Plane Symmetric Gravitational Fields in (D+1)-dimensional General Relativity3
Dynamical Diagnostics of Anisotropic Barrow Holographic Dark Energy Models with Massive Scalar Fields3
Plane-Symmetric Universe in the Presence of String Clouds Coupled with the Perfect Fluid in f(R,T) Gravity3
Total C+N+O Abundances in the Atmospheres of Red Giants of Different Metallicities3
Temperature Effects in the Proto Neutron Star Phase of PSR J0740+66202
Features of the Magnetic Field Behavior of the Ae/Be Star HD1900732
Photometric Study and Orbital Solution for Some Newly Discovered Eclipsing Binary Systems2
Effect of the Interaction Between Hyperons on the Moment of Inertia of the Proto Neutron Stars2
Re-Examining Berman’s Parametrization of the Hubble Parameter in the Context of Late-Time Acceleration2
Modified Tsallis Holographic Dark Energy2
Variation of Doppler Velocities and D3 Spicule Half-Widths2
Correction to: Induced Electromagnetic Radiation from a Charged Cloud in a Plane Gravitational Wave2
Photometric Study of the Asynchronous Polar IGR J19552+0044 in 2019-20222
Special Properties of Magnetic O-Type Star HD1494382
Correction to: A Search for New Dwarf Galaxies Outside the Nearby Groups2
Photometric and Spectral Studies of a Group of Wolf-Rayet Galactic Stars. II. WC and WO Sequences2
The Mysterious Radcliffe Wave2
Observational Constraining of Viscous Ghost Dark Energy in f(R,T) Gravity2
New M-type Periodic Variables of Catalina Sky Survey Database2
Fermionic Vacuum Stresses in Models with Toroidal Compact Dimensions2
Evolution of Spectrum Lines in an Inhomogeneous Atmosphere Illuminated by Nonstationary Energy Sources2
Novel Planetary Signatures from the Dark Universe2
Structure of the Magnetic Field of the Star HD133880 (Si)2
Correction to: Electromagnetic Radiation from a Relativistic Jet Induced by a Plane Gravitational Wave2
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