small pl CAMK logo

Strona główna

» Z naszych badań

 archiwum | rss

 

Journal Club i Wednesday Colloquia odbywają się w wersji hybrydowej lub wyłącznie online (zależnie od prelegenta). Więcej...o dostępie online

Najbliższe seminaria


Wednesday Colloquium 08.10.2025

Jarosław Duda

Do astronomical objects create also negative radiation pressure?
Journal Club 13.10.2025

Sudhagar Suyamprakasam

GWTC-4.0 catalog paper
SPOTKANIA z ASTRONOMIĄ 27.10.2025

Przemysław Mróz

Czy ciemna materia we Wszechświecie składa się czarnych dziur?

» Aktualności

 archiwum | rss

» Niedawne publikacje w arXiv

 archiwum
arXiv:2510.03766[pdf, other]
Formation and growth of intermediate-mass black holes in dense star clusters: Lessons from N-body and MOCCA Monte Carlo Simulations
Comments:4 pages, 2 figures, 1 table. To appear in the Proceedings of IAU Symposium 398 and MODEST-25: "Compact Objects and Binaries in Dense Stellar Systems" (Seoul, South Korea, June 2025)
arXiv:2510.02751[pdf, other]
Self-lensing binaries in globular clusters -- predictions for ELT
Comments:12 pages, 8 figures, submitted to A&A
arXiv:2510.02858[pdf, other]
PINNGraPE: Physics Informed Neural Network for Gravitational wave Parameter Estimation
Comments:4 pages, 2 figures. Proceedings contribution to Journal of Physics: Conference Series for the 24th International Conference on General Relativity and Gravitation (GR24) and the 16th Edoardo Amaldi Conference on Gravitational Waves (Amaldi16)
arXiv:2510.04746[pdf, other]
Characterizing the variability of a sample of massive stars in eclipsing binaries
Comments:10 pages, 3 figures, 2 tables
arXiv:2509.24114[pdf, other]
Telling apart black holes and naked singularities with trajectories of massive particles
Comments:8 pages, 10 figures, submitted to MNRAS
arXiv:2510.01045[pdf, other]
Carbon and nitrogen as indicators of stellar evolution and age. A homogeneous sample of 44 open clusters from the Gaia-ESO Survey
Comments:10 pages, 7 figures
arXiv:2510.05017[pdf, other]
Exploring Low-Amplitude Variability in First Overtone Cepheids with TESS
Comments:Accepted for publication in A&A