activity
20162025
most citedA scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the Main Sequence to planets

55 citations · 160 across the 12 of their papers we have counts for

collaborators

16 papers

astro-ph.GA20229 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…

astro-ph.SR202155 cited

A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the Main Sequence to planets

P. Leto, C. Trigilio, J. Krticka +20

In this paper, we present the analysis of incoherent non-thermal radio emission from a sample of hot magnetic stars, ranging from early-B to early-A spectral type. Spanning a wide…

astro-ph.GA202114 cited

Evolutionary Map of the Universe (EMU):Compact radio sources in the SCORPIO field towards the Galactic plane

S. Riggi, G. Umana, C. Trigilio +26

We present observations of a region of the Galactic plane taken during the Early Science Program of the Australian Square Kilometre Array Pathfinder (ASKAP). In this context, we ob…

astro-ph.GA20206 cited

A warm molecular ring in AG Car: composing the mass-loss puzzle

C. Bordiu, F. Bufano, L. Cerrigone +9

We present APEX observations of CO J=3-2 and ALMA observations of CO J=2-1, 13CO J=2-1 and continuum toward the galactic luminous blue variable AG Car. These new observations revea…

astro-ph.HE202014 cited

New high-frequency radio observations of the Cygnus Loop supernova remnant with the Italian radio telescopes

S. Loru, A. Pellizzoni, E. Egron +19

Supernova remnants (SNRs) represent a powerful laboratory to study the Cosmic-Ray acceleration processes at the shocks, and their relation to the properties of the circumstellar me…

astro-ph.SR2020

The auroral radio emission of the magnetic B-type star rho OphC

P. Leto, C. Trigilio, C. S. Buemi +19

The non-thermal radio emission of main-sequence early-type stars is a signature of stellar magnetism. We present multi-wavelength (1.6-16.7 GHz) ATCA measurements of the early-type…