110 citations · 418 across the 10 of their papers we have counts for
10 papers
The unidentified PeV source LHAASO J2108+5157: A microquasar remnant?
Josep Mart\'ı, Pedro L. Luque-Escamilla, Leandro Abaroa +4
Context. LHAASO~J2108+5157 is one of the most intriguing Galactic ultra-high-energy -ray sources. It is detected up to hundreds of TeV but lacks a clear counterpart at lower fre…
X-ray study of bow shocks in runaway stars
M. De Becker, M. V. del Valle, G. E. Romero +2
Massive runaway stars produce bow shocks through the interaction of their winds with the interstellar medium, with the prospect for particle acceleration by the shocks. These objec…
An investigation into the fraction of particle accelerators among colliding-wind binaries. Towards an extension of the catalogue
M. De Becker, P. Benaglia, G. E. Romero +1
Particle-accelerating colliding-wind binaries (PACWBs) are multiple systems made of early-type stars able to accelerate particles up to relativistic velocities. The relativistic pa…
E-BOSS: An Extensive stellar BOw Shock Survey. II. Catalogue second release
C. S. Peri, P. Benaglia, N. L. Isequilla
Context. Stellar bow shocks have been studied not only observationally, but also theoretically since the late 1980s. Only a few catalogues of them exist. The bow shocks show emissi…
Evidence of non-thermal X-ray emission from HH 80
J. Lopez-Santiago, C. S. Peri, R. Bonito +4
Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km/s, creating strong shocks when int…
High resolution radio emission from RCW 49/Westerlund 2
Paula Benaglia, Baerbel Koribalski, Cintia S. Peri +4
RCW49 and its ionizing cluster form an extensive, complex region, widely studied at IR and optical wavelengths. Molonglo 843 MHz and ATCA data at 1.4 and 2.4 GHz showed two shells.…