activity
20162025
most citedNew insights in the HII region G18.88-0.49: hub-filament system and accreting filaments

37 citations · 131 across the 12 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2025★ 3 cited

Probing the detectability of electromagnetic signatures from Galactic isolated black holes

Javier Rodrigo Martinez, Valenti Bosch-Ramon, Florencia Laura Vieyro +1

Context: A large number of isolated black holes (IBHs) are expected to populate the Galaxy. However, only one has been confirmed by the analysis of a microlensing event, and no con…

astro-ph.HE2023★ 5 cited

The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3

Jun Yang, Federico García, Santiago del Palacio +6

Cygnus X-3 is a high-mass X-ray binary with a compact object accreting matter from a Wolf-Rayet donor star. Recently, it has been revealed by the Imaging X-ray Polarimetry Explorer…

astro-ph.HE2022★ 5 cited

Non-thermal emission in hyper-velocity and semi-relativistic stars

J. R. Martinez, S. del Palacio, V. Bosch-Ramon +1

Context. There is a population of runaway stars that move at extremely high speeds with respect to their surroundings. The fast motion and the stellar wind of these stars, plus the…

astro-ph.HE2020★ 7 cited

The high-energy emission from HD~93129A near periastron

S. del Palacio, F. García, D. Altamirano +12

We conducted an observational campaign towards one of the most massive and luminous colliding wind binaries in the Galaxy, HD~93129A, close to its periastron passage in 2018. Durin…

astro-ph.HE2017★ 22 cited

Gamma rays from clumpy wind-jet interactions in high-mass microquasars

V. M. de la Cita, S. del Palacio, V. Bosch-Ramon +3

The stellar winds of the massive stars in high-mass microquasars are thought to be inhomogeneous. The interaction of these inhomogeneities, or clumps, with the jets of these object…

astro-ph.HE2016★ 24 cited

A model for the non-thermal emission of the very massive colliding-wind binary HD 93129A

Santiago del Palacio, Valentí Bosch-Ramon, Gustavo E. Romero +1

The binary stellar system HD 93129A is one of the most massive known binaries in our Galaxy. This system presents non-thermal emission in the radio band, which can be used to infer…