activity
20202026
most citedX-ray spectropolarimetric characterization of the Z-source GX 340+0 in the normal branch

4 citations · 4 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

mm-jets in the multi-messenger era

Karri I. I. Koljonen, Thomas D. Russell, Britton Jeter +16

Jets and outflows operate across the full cosmic mass scale from young stellar objects (YSOs) and X-ray binaries (XRBs) to active galactic nuclei (AGN), gamma-ray bursts (GRBs), an…

astro-ph.HE2026

XMM-Newton Resolves Parsec-scale X-ray Jets in the PeVatron Microquasar V4641 Sgr

Naomi Tsuji, Caterina Tresoldi, Kaya Mori +34

The microquasar V4641 Sagittarii (V4641 Sgr) has recently been established as one of the most powerful Galactic PeV cosmic-ray accelerators (PeVatrons) through the detection of deg…

astro-ph.HE2026

Connecting radio pulsars, magnetars, and XDINSs in a unified evolutionary framework using simulation-based inference

Michele Ronchi, Celsa Pardo-Araujo, Vanessa Graber +7

Understanding the Galactic population of isolated neutron stars within a unified framework provides key insights into their birth properties, evolutionary pathways, and the connect…

astro-ph.HE2026

A candidate proton cyclotron feature in the ultraluminous X-ray source NGC 4656 ULX-1

Nelson Cruz-Sanchez, Enzo A. Saavedra, Federico A. Fogantini +6

Ultraluminous X-ray sources represent extreme super-Eddington accretion regimes, and a subset is now known to host highly magnetized neutron stars. However, direct observational pr…

astro-ph.HE2025★ 4 cited

X-ray spectropolarimetric characterization of the Z-source GX 340+0 in the normal branch

Fabio La Monaca, Alessandro Di Marco, Francesco Coti Zelati +11

This study presents an X-ray spectropolarimetric characterisation of the Z-source GX 340+0 during the normal branch (NB) and compares it with that obtained for the horizontal branc…

astro-ph.EP2020

Stability of Planetary Motion in Binary Star Systems

Roberto Capuzzo-Dolcetta, Giovanni De Cesare, Alessio Marino

We considered the problem of stability for planets of finite mass in binary star systems. We selected a huge set of initial conditions for planetary orbits of the S-type, to perfor…