activity
20202026
most citedAU-scale radio imaging of the wind collision region in the brightest and most luminous non-thermal colliding wind binary Apep

17 citations · 27 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Investigating particle acceleration in the Wolf-Rayet bubble NGC 2359

Anindya Saha, Anandmayee Tej, Santiago del Palacio +4

Massive stars have been proposed as candidates to be major factories of Galactic cosmic rays (GCRs). However, this claim lacks enough empirical evidence, especially for isolated st…

astro-ph.HE2025★ 2 cited

EWOCS-IV: 1Ms ACIS Chandra observation of the supergiant B[e] star Wd1-9

K. Anastasopoulou, M. G. Guarcello, J. J. Drake +21

Supergiant B[e] (sgB[e]) stars are exceptionally rare objects, with only a handful of confirmed examples in the Milky Way. The evolutionary pathways leading to the sgB[e] phase rem…

astro-ph.IM2025★ 8 cited

Robust Binding Energy Distribution Sampling on Amorphous Solid Water Models. Method testing and validation with NH3, CO and CH4

Maria Groyne, Benoît Champagne, Cedric Baijot +1

This work aims to develop a method based on a structurally reliable ice model and a statistically and physico-chemically robust approach for BE distribution inference, with the aim…

astro-ph.HE2024

EWOCS-II: X-ray properties of the Wolf-Rayet stars in the young Galactic super star cluster Westerlund 1

K. Anastasopoulou, M. G. Guarcello, E. Flaccomio +20

We present the most comprehensive and deepest X-ray study to date of the properties of the richest Wolf-Rayet (WR) population observed in a single stellar cluster, Westerlund 1 (Wd…

astro-ph.SR2023

A preliminary timing analysis of two intermediate polars: UU Col and Swift J0939.7-3224

Nikita Rawat, J. C. Pandey, Arti Joshi +2

We present the preliminary timing analysis of confirmed intermediate polar UU Col and possible intermediate polar Swift J0939.7-3224 in the optical band with the help of long-term,…

astro-ph.SR2020★ 17 cited

AU-scale radio imaging of the wind collision region in the brightest and most luminous non-thermal colliding wind binary Apep

B. Marcote, J. R. Callingham, M. De Becker +5

The recently discovered colliding-wind binary (CWB) Apep has been shown to emit luminously from radio to X-rays, with the emission driven by a binary composed of two Wolf-Rayet (WR…