collaborators

8 papers

astro-ph.SR2026

Star Planet Interactions

Arghyadeep Paul, Kristina Kislyakova, Manuel Güdel +13

Star-planet interactions (SPIs) describe the continuous exchange of energy, momentum, and mass between exoplanets and their host stars through radiative, tidal, magnetic, and parti…

astro-ph.HE2026

Planets in Pulsar Winds

T. Kaister, S. Andrés Joya Méndez, P. Marmat +4

Planets around pulsars were the first discovered exoplanets, found thanks to the extremely precise pulsar timing. Here we suggest that they could also be found through the radio em…

astro-ph.HE2026

Strange quark star II: the minimal and maximal gravitational mass and the Keplerian configuration

Fatemeh Kayanikhoo, Mateusz Kapusta, Miljenko Čemeljić +2

We employ the MIT bag model with density-dependent bag constant for the equation of state (EOS) to estimate the gravitational mass and Keplerian frequency of rapidly rotating stran…

astro-ph.HE2026

Strange quark star I: the maximum gravitational mass and deformation of magnetized spinning model

Fatemeh Kayanikhoo, Mateusz Kapusta, Miljenko Čemeljić +1

We investigate the structural parameters of strange quark stars (SQS) under the influence of strong magnetic fields and varying rotational frequencies. The equation of state is com…

astro-ph.HE2025

Binary black holes in magnetized AGN disks

Raj Kishor Joshi, Aryan Bhake, Biswajit Banerjee +7

Stellar-mass binary black hole (BBH) mergers occurring within the disks of active galactic nuclei (AGN) are promising sources for gravitational waves detectable by the LIGO, Virgo,…

astro-ph.HE2025

Magnetic precession as a model for QPOs in PULXs: flat-top noise ULXs are different

Miljenko Čemeljić, Włodek Kluźniak, Sukalpa Kundu

Context. Several instances of low frequency Quasi-Periodic Oscillations (QPOs) have been reported in ultraluminous X-ray sources (ULXs), including three in pulsating ones (PULXs) t…