- https://doi.org/10.1134/s1063772925701999
Reasons for the Slow Apsidal Rotation of the Massive Eclipsing Star V1141 Cas
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Translate Article Take Notes Reasons for the Slow Apsidal Rotation of the Massive Eclipsing Star V1141 Cas
ReferencesShowing 10 of 29 papersTransformations from Theoretical Hertzsprung-Russell Diagrams to Color-Magnitude Diagrams: Effective Temperatures, B-V Colors, and Bolometric Corrections The Absolute Calibration of the HR Diagram: Fundamental Effective Temperatures and Bolometric Corrections Misaligned spin and orbital axes cause the anomalous precession of DI Herculis Eclipsing System PS UMa: Evolutionary Status and Physical Parameters of the Components Multiplicity and apsidal motion in the eclipsing binary EQ Boo Rediscussion of eclipsing binaries. XIII - DI Herculis, a B-type system with an eccentric orbit UBVRIPHOTOMETRIC STANDARD STARS AROUND THE CELESTIAL EQUATOR: UPDATES AND ADDITIONS Estimation of parameter errors in inverse problems. Determining limb-darkening coefficients in classical eclipsing systems Absolute Parameters and Apsidal Motion of the Eclipsing System V501 Mon On the relativistic motion of the periastron in the eclipsing binary system DI Herculis
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