Vol. 50, No. 9, 2024
Prospects for Measuring the Post-Newtonian \(\boldsymbol{\gamma}\) Parameter Using Two Satellites Equipped with Highly Stable Atomic Clocks and a Doppler Compensation System
p. 537 abstract
Parameters of the Possible Companion of the Neutron Star toward the Supernova Remnant G315.4–2.30
p. 550 abstract
Models of Mira Variables of the Large Magellanic Cloud
p. 561 abstract
Radial Velocities of Narrow Emission Line Components in the Spectra of T Tauri Stars
p. 571 abstract
Magnetic Flux Ropes with a Current Shell As Flaring Solar Structures
p. 584 abstract