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Should we expect further acceleration of the Earth’s rotation in the coming years?
Malkin Z.
Time structure of the average rotation measure for accretion disk in shearing box approximation
Buldakov M., Andrianov A.
VARIATION OF GLOBAL AND LOCAL FLOWS IN THE SOLAR CONVECTION ZONE DURING ACTIVITY CYCLES 24 AND 25
Getling A., Kosovichev A.
THE ROLE OF MERIDIONAL CIRCULATION IN THE FORMATION OF CLASSICAL BE-STARS
Staritsin E.
Equilibrium figures of two liquid masses with synchronous rotation. Dynamics of a double asteroid (190166) 2005 UP156
Kondratyev B.
MODERN ESTIMATES OF THE MASS OF THE MILKY WAY
Bobylev V., Baykova A.
Determination of dynamic and physical characteristics of near-Earth asteroids based on observations from 2022–2023
Kuznetsov Е., Wiebe Y., Glamazda D., Kaiser G., Krushinsky V., Kryuchkov M., Naroenkov S., Perminov A.
Spot and flare activity of single G5 III IV giant HD 199178 from TESS observations
Savanov I., Tarasenkov A., Dmitrienko E.
New formula for the angular velocity of rotation of liquid equilibrium figures
Kondratyev B.
Tayler instability of magnetic field as possible reason for the period changes in Ap star 56 Ari
Potravnov I., Kitchatinov L.
V957 Cep is a Zero-Age Eclipsing System
Volkov I., Naroenkov S., Kravtsova A.
Kinematics of stars with radially elongated orbits located within 100 pc from the sun
Postnikova E., Chupina N., Vereshchagin S.
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