Vol. 67, No. 11, 2023
Modern Stellar Astronomy 2022
p. 1065 abstract
Evolution of the X-ray Binary System Sco X-1
p. 1074 abstract
Interaction of the Exoplanet Hat–P–11b with Stellar Wind
p. 1091 abstract
On the Possibility to Estimate the Orbital Eccentricity of a Binary System with an Exoplanet from a Transit Light Curve
p. 1096 abstract
NO Biomarker: Transmission and Emission Methods for Its Potential Detection in Exoplanet Atmospheres with Spektr-UF (WSO-UV)
p. 1123 abstract
The Near Infrared and Optical Photometric Activity of V517 Cyg
p. 1139 abstract
Scale-Invariant Mode in Collisionless Spherical Stellar Systems
p. 1156 abstract
Next Generation Gravity Missions: Studying the Possibilities of Multiple Constellations
p. 1165 abstract
Parameters of Radio Pulsars at Different Distances from the “Death Line”
p. 1177 abstract
Estimation of the Pulsar Braking Index Using the Evolution of the Rotational Kinetic Energy Loss Rate. Testing on the Crab Pulsar
p. 1187 abstract
A Planet or Primordial Black Hole in the Outer Region of the Solar System and the Dust Flow near Earth’s Orbit
p. 1193 abstract
On the Question of Localizing the Birthplaces of Coronal Mass Ejections on the Sun
p. 1205 abstract
Statistics of Thermal Plasma Parameters and Non-Thermal X-Ray Spectra of Solar Flares with Helioseismic Response
p. 1216 abstract
Gravitational Capture as a Possible Scenario Origin of the Moon
p. 1236 abstract
The Role of Oblateness in Shaping Stability and Zero Velocity Curves in the Perturbed Restricted Three-Body Problem
p. 1251 abstract