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Temporal Equivalence Principle: Suppressed Density Scaling in Globular Cluster Pulsars — 199 cluster vs 351 field millisecond pulsars show a +0.61 dex controlled spin-down residual (5.8σ) and suppressed density scaling (Γ=0.39±0.08 vs Newtonian 0.72), while 20-cluster CMC N-body realizations overpredict the excess by 3.2× (8.6σ).
An astronomical data analysis repository focused on the open cluster NGC 2099 (Messier 37). This project studies and compares astrometric and photometric data across the Gaia DR2, EDR3, and DR3 releases to analyze cluster properties and catalog variations.
Android globus coelestis (celestial globe) and interactive calendar with Zodiac signs and timepiece covering the Solar System in the entire observable universe.
This aim of this project is to analyze globular star clusters in the Milky Way, in order to understand their dynamics. The conducted study examined the properties that affect the central velocity dispersion, their impact and the correlations between them.