activity
20022026
most citedStar formation triggered by SN explosions: an application to the stellar association of Pictoris

39 citations · 51 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

GRMHD accretion beyond the black hole paradigm: Light from within the shadow

Saurabh, Maciek Wielgus, Parth Bambhaniya +3

We present the first three-dimensional general relativistic magnetohydrodynamic simulation of sustained accretion onto a horizonless singularity in which matter reaches the central…

gr-qc2025

Time Delay of Pulsar Signals in Astrophysical Black Hole Spacetimes

Parth Bambhaniya, Viraj Kalsariya, Saurabh +4

In this paper, we investigate the fully relativistic time delay of pulsar signals propagating in the vicinity of a rotating black hole and its potential mimickers, including a defo…

astro-ph.HE2025

Particle acceleration by turbulent-driven magnetic reconnection and the production of gamma-rays and neutrinos in AGNs

E. M. de Gouveia Dal Pino, J. C. Ramirez-Rodriguez, T. Medina-Torrejon +2

3D Magnetohydrodynamic (MHD) resistive simulations have highlighted the significance of ubiquitous turbulence to drive fast reconnection. It has been demonstrated that particle acc…

astro-ph.HE2024★ 7 cited

Galactic transient sources with the Cherenkov Telescope Array Observatory

Cherenkov Telescope Array Observatory Consortium

A wide variety of Galactic sources show transient emission at soft and hard X-ray energies: low- and high-mass X-ray binaries containing compact objects, isolated neutron stars exh…

astro-ph.CO2012

Characterizing the magnetic field in the intracluster medium

M. S. Nakwacki, E. M. de Gouveia Dal Pino, G. Kowal +1

During structure formation, energetic events and random motions of the hot gas residing inside galaxy clusters (the intracluster medium, ICM) generate turbulent motions. Radio diff…

astro-ph2008

Flux transport solar dynamo models, current problems and possible solutions

G. Guerrero, E. M. de Gouveia Dal Pino

The sunspot solar cycle has been usually explained as the result of a dynamo process operating in the sun. This is a classical problem in Astrophysics that until the present is not…