activity
19992025
most citedThe radio lighthouse CU Virginis: the spindown of a single main sequence star

42 citations · 88 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2025

Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A

KM3NeT Collaboration, O. Adriani, A. Albert +278

Context: The detection of the highest energy neutrino observed to date by KM3NeT, with an estimated energy of 220 PeV, opens up new possibilities for the study and identification o…

astro-ph.HE2025

A semi-coherent search for optical pulsations from Scorpius X-1

Riccardo La Placa, Alessandro Papitto, Giulia Illiano +14

The emission of continuous gravitational waves (CWs) possibly explains why pulsars spinning with a period shorter than a millisecond have not been observed so far. Neutron stars ac…

nucl-ex2025

Direct proton transfer on Ar supports the presence of a charge density bubble linked to a novel nuclear structure below Ca

Daniele Brugnara, Andrea Gottardo, Marlene Assiè +76

The Ar(He,d)K reaction was performed in inverse kinematics using a radioactive Ar beam produced by the SPIRAL1 facility at GANIL and a cryogenic He t…

astro-ph.SR2024★ 2 cited

Gravity's role in taming the Tayler instability in red giant cores

Domenico G. Meduri, Rainer Arlt, Alfio Bonanno +1

The stability of toroidal magnetic fields in radiative stellar interiors is a key open problem in astrophysics. We investigate the Tayler instability of purely toroidal fields $B_ϕ…

astro-ph.GA2015★ 1 cited

The normal chemistry of multiple stellar populations in the dense globular cluster NGC 6093 (M 80)

E. Carretta, A. Bragaglia, R. G. Gratton +6

We present the abundance analysis of 82 red giant branch stars in the dense, metal-poor globular cluster NGC 6093 (M 80), the largest sample of stars analyzed in this way for this…

astro-ph.SR2011

EVLA observations of the nebula around G79.29+0.46

G. Umana, C. S. Buemi, C. Trigilio +5

We have observed the radio nebula surrounding the Galactic LBV candidate G79.29+0.46 with the EVLA at 6 cm. These new radio observations allow a morphological comparison between th…