collaborators

5 papers

astro-ph.GA2026

A Kiloparsec-Scale Stellar Cavity in the Center of Abell402-BCG May be Caused by Dynamic Interactions with an Ultramassive Black Hole

Michael McDonald, Gourav Khullar, David Lagattuta +18

We present new observations from JWST NIRCam that reveal a striking kpc-wide cavity in the stellar distribution of the central galaxy in the cluster Abell402. Supporting data from…

astro-ph.SR2025

Young M dwarfs flare activity model: Towards better exoplanetary atmospheric characterisation

E. Mamonova, A. F. Kowalski, K. Herbst +2

Context. Stellar flares can significantly influence the atmospheres and habitability of orbiting exoplanets, especially around young and active M dwarfs. Understanding the temporal…

astro-ph.EP2025

Planets similar in size are often dissimilar in interior

E. Mamonova, Y. Shan, P. Hatalova +1

Recent works have found evidence of significant intrasystem uniformity in planet properties such as radius, mass, and orbital spacing, collectively termed 'peas in a pod' trends. I…

astro-ph.SR2025

Flare frequency in M dwarfs belonging to Young Moving Groups

E. Mamonova, Y. Shan, A. F. Kowalski +1

Context. M stars are preferred targets for studying terrestrial exoplanets, for which we hope to obtain their atmosphere spectra in the next decade. However, M dwarfs have long bee…

astro-ph.EP2025

The current cratering rate on the regular satellites of Jupiter, Saturn, and Uranus

R. Brasser, E. W. Wong, S. C. Werner

We aim to compute the impact rates for objects with a diameter of 1 km onto the regular satellites of Jupiter, Saturn and Uranus using our latest dynamical simulations of the evolu…