Works matching IS 10637737 AND DT 2022 AND VI 48 AND IP 3
Results: 7
Application of the Hori–Deprit Method to the Analysis of the Cosmogonic Evolution of Weakly Perturbed Planetary Systems.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 194, doi. 10.1134/S1063773722030045
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Toroidal Magnetic Chamber "Tokamak" in the Solar Atmosphere: Confinement and Flare Magnetic Energy Release.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 185, doi. 10.1134/S1063773722030057
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Atomic Data on Inelastic Processes in Boron–Hydrogen Collisions.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 178, doi. 10.1134/S106377372203001X
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Estimation of Galactic Spiral Density Wave Parameters Based on the Velocities of OB2 Stars from the Gaia EDR3 Catalogue.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 169, doi. 10.1134/S1063773722020025
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Type Ibn Supernova SN 2010al: Powerful Mass Loss Half Year Prior to the Explosion.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 163, doi. 10.1134/S1063773722030033
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Forced Photometry for Pan-STARRS1 Objects Based on WISE Data.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 153, doi. 10.1134/S1063773722030021
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Young Star-Forming Complexes in the Ring of the S0 Galaxy NGC 4324.
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- Astronomy Letters, 2022, v. 48, n. 3, p. 139, doi. 10.1134/S1063773722020049
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- Article