activity
20012026
most citedA change in the optical polarization associated with a gamma-ray flare in the blazar 3C 279

334 citations · 3.4k across the 83 of their papers we have counts for

collaborators

83 papers

astro-ph.SR2026

Discovery of sulfur oxides in the ejecta of a B[e] supergiant

C. Bordiu, J. Ricardo Rizzo, D. Navarro-Almaida +12

B[e] supergiants represent a rare class of luminous, evolved massive stars surrounded by dusty circumstellar disks. Since their intense UV fields were long thought to sterilize the…

astro-ph.SR2026

Coherent and Incoherent Emission from the Ordered Magnetospheres of Low-Mass Stars, UCDs, and Massive Stars

Francesco Cavallaro, Paolo Leto, Barnali Das +15

Massive early-type (B/A) stars and ultracool dwarfs (UCDs) represent two distinct regimes in which ordered, large-scale magnetospheres are observed. In rapidly rotating massive sta…

astro-ph.SR2024

The distance to CRL 618 through its radio expansion parallax

L. Cerrigone, G. Umana, C. Trigilio +9

CRL 618 is a post-AGB star that has started to ionize its ejecta. Its central HII region has been observed over the last 40 years and has steadily increased in flux density at radi…

astro-ph.SR2023★ 3 cited

The rich molecular environment of the luminous blue variable star AFGL 2298

J. R. Rizzo, C. Bordiu, C. Buemi +6

We investigated the molecular environment of AFGL 2298, an obscured Galactic Luminous blue variable (LBV) star which hosts a highly structured circumstellar environment with hints…

astro-ph.EP2023★ 6 cited

Star-Planet Interaction at radio wavelengths in YZ Ceti: Inferring planetary magnetic field

Corrado Trigilio, Ayan Biswas, Paolo Leto +13

In exoplanetary systems, the interaction between the central star and the planet can trigger Auroral Radio Emission (ARE), due to the Electron Cyclotron Maser mechanism. The high b…

astro-ph.GA2022★ 9 cited

First detection of silicon-bearing molecules in Car

C. Bordiu, J. R. Rizzo, F. Bufano +11

We present ALMA band 6 observations of the luminous blue variable Eta Car, obtained within the ALMAGAL program. We report SiO J=5-4, SiS J=12-11 and SiN N=5-4 emission in the equat…