Works matching IS 10637729 AND DT 2024 AND VI 68 AND IP 5
Results: 8
Microstructure in Radio Emission of the Pulsar B1133+16 at a Frequency of 111 MHz.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 514, doi. 10.1134/S1063772924700471
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Metallicity and Kinematics of the Circumsolar Stellar Population of the Galaxy.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 527, doi. 10.1134/S1063772924700483
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Constructing an Entropy-Force Model of the Expansion of the Universe Due to Gravitationally Induced Production of Dark Matter.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 499, doi. 10.1134/S106377292470046X
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Determination of the Parameters of the Gravitational Field of the Earth by Gradiometric Measurements in the Earth's Geocentric Coordinate System.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 489, doi. 10.1134/S1063772924700458
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V957 CEP—A Zero-Age Eclipsing System.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 472, doi. 10.1134/S1063772924700446
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Investigation of H<sub>2</sub>O and OH Masers in the Region of Formation of a Young High-Mass Stellar Object (S255 NIRS 3).
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- Astronomy Reports, 2024, v. 68, n. 5, p. 453, doi. 10.1134/S1063772924700434
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Gas-Dynamical Model of Accretion on a Neutron Star with Viscosity and the Influence of Large-Scale Vortices on the Transmission of Angular Momentum.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 438, doi. 10.1134/S1063772924700422
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On the Generalized Kepler Problem under the Effect of Outer Third-Body Perturbation.
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- Astronomy Reports, 2024, v. 68, n. 5, p. 429, doi. 10.1134/S1063772924700410
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- Article