activity
20112026
most citedRelativistic Jets Shine through Shocks or Magnetic Reconnection?

333 citations · 4.2k across the 122 of their papers we have counts for

collaborators
Showing 2017Show all

6 papers · 1 filter

astro-ph.HE2017★ 16 cited

Identification of two new HMXBs in the LMC: a 2013 s pulsar and a probable SFXT

G. Vasilopoulos, C. Maitra, F. Haberl +2

We report on the X-ray and optical properties of two high-mass X-ray binary systems located in the Large Magellanic Cloud (LMC). Based on the obtained optical spectra, we classify…

astro-ph.HE2017★ 18 cited

X-ray mapping of the stellar wind in the binary PSR J2032+4127/MT91 213

M. Petropoulou, G. Vasilopoulos, I. M. Christie +2

PSR J2032+4127 is a young and rapidly rotating pulsar on a highly eccentric orbit around the high-mass Be star MT91 213. X-ray monitoring of the binary system over a 4000 day…

astro-ph.HE2017★ 31 cited

Plasmoid statistics in relativistic magnetic reconnection

M. Petropoulou, I. M. Christie, L. Sironi +1

Plasmoids, quasi-spherical regions of plasma containing magnetic fields and high-energy particles, are a self-consistent by-product of the reconnection process in the relativistic…

astro-ph.HE2017★ 12 cited

Collapsar Gamma-Ray Bursts: how the luminosity function dictates the duration distribution

Maria Petropoulou, Rodolfo Barniol Duran, Dimitrios Giannios

Jets in long-duration -ray bursts (GRBs) have to drill through the collapsing star in order to break out of it and produce the -ray signal while the central engine is still a…

astro-ph.HE2017★ 55 cited

Point-source and diffuse high-energy neutrino emission from Type IIn supernovae

Maria Petropoulou, Stefan Coenders, Georgios Vasilopoulos +2

Type IIn supernovae (SNe), a rare subclass of core collapse SNe, explode in dense circumstellar media that have been modified by the SNe progenitors at their last evolutionary stag…

astro-ph.HE2017★ 1 cited

Radio Emission from Sgr A*: Pulsar Transits Through the Accretion Disc

Ian Christie, Maria Petropoulou, Petar Mimica +1

Radiatively inefficient accretion flow models have been shown to accurately account for the spectrum and luminosity observed from Sgr A* in the X-ray regime down to mm wavelengths.…