activity
20152026
most citedA shared accretion instability for black holes and neutron stars

38 citations · 181 across the 35 of their papers we have counts for

collaborators
Showing 2026 · astro-ph.HEShow all

11 papers · 2 filters

astro-ph.HE2026

Phase-resolved X-ray spectroscopy of the Vela pulsar with NICER observations

E. Zubieta, F. García, S. del Palacio +2

PSR J0835-4510 (a.k.a. the Vela pulsar) is the best studied pulsar in the Southern hemisphere given its high radio brightness and large glitch activity. However, its X-ray brightne…

astro-ph.HE2026

The influence of free-free absorption on the radio spectrum of Particle-Accelerating Colliding-Wind Binaries

Michaël De Becker, Agustina Belen Blanco, Mathilde Tasseroul +4

The study of massive stars in binary and higher-multiplicity systems that participate in particle acceleration is a key topic at the crossroads of massive star physics, shock physi…

astro-ph.HE2026

Radio Emission with Dust: A Bow-Shock Interpretation for the TDE Candidate AT 2019avd

Shuyuan Wei, Yanan Wang, Guobin Mou +5

Forward shocks produced by interactions between a single ejected blob and the circumnuclear medium (CNM) around a supermassive black hole are widely invoked to explain radio emissi…

astro-ph.HE2026

Single-pulse reanalysis of the 2024 Vela glitch and new observations of PSR~J04374715 and PSR~J16444559

Carlos O. Lousto, Ruby Shrestha, Ezequiel Zubieta +6

The Pulsar Monitoring in Argentina (PuMA) collaboration systematically monitors southern glitching pulsars, maintaining high-cadence single-pulse records of the Vela pulsar. We pre…

astro-ph.HE2026

First fast radio burst search campaign at the Argentine Institute of Radio Astronomy

Carlos O. Lousto, Harsh Prajapati, Ezequiel Zubieta +7

Fast radio bursts (FRBs) are intense millisecond-duration radio transients of extragalactic origin whose physical nature remains under active investigation, and which also serve as…

astro-ph.HE2026

Enabling population studies on wind-driven Galactic binary systems

B. Marcote, P. Benaglia, V. Bosch-Ramon +8

Galactic binaries driven by stellar wind shocks, such as colliding wind binaries (CWBs) and gamma-ray binaries (gBs), harbor one of the most efficient particle acceleration engines…

astro-ph.HE2026

Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars

Emma Kun, Imre Bartos, Claudio Ricci +5

The origin of high-energy astrophysical neutrinos remains a key open question in multimessenger astrophysics. A correlation between unabsorbed hard X-ray and high-energy neutrino l…

astro-ph.HE2026

The Emerging Population of High-energy Emitting Radio Galaxies

G. Bruni, V. S. Paliya, D. J. Saikia +22

High-energy emission from radio galaxies provides a unique laboratory to study the connection between accretion, jet formation, and particle acceleration in active galactic nuclei…

astro-ph.HE2026

The Millimeter/X-ray Relation in Rapidly Accreting Supermassive Black Holes at

Sophie M. Venselaar, Claudio Ricci, Santiago Del Palacio +12

A tight correlation between nuclear millimeter and X-ray emission has recently been found in nearby () and low-Eddington ratio () radio-quiet Active Ga…

astro-ph.HE2026

Upstream neutrino production and delayed jet emission in the blazar GB6 J1542+6129

Emma Kun, Imre Bartos, Breshna Hadi +7

We present a multimessenger case study of the blazar GB6 J1542+6129, examining whether its multiwavelength behavior is consistent with neutrino production in a compact region near…

astro-ph.HE2026

Giant radio pulses in the magnetar XTE J1810-197 detected with the IAR's telescopes

S. B. Araujo Furlan, G. E. Romero, E. Zubieta +4

[...] We observed XTE J1810-197 between 29 September 2022 and 14 July 2023 with the radio telescopes at the Argentine Institute of Radioastronomy (IAR). We searched for single puls…