activity
20112021
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 1.3k across the 29 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2021★ 4 cited

LBV phenomenon and binarity: The environment of HR Car

A. Mehner, S. Janssens, C. Agliozzo +7

Luminous blue variable stars (LBVs) are of great interest in massive-star evolution as they experience very high mass-loss episodes within short periods of time. HR Car is a famous…

astro-ph.SR2021★ 8 cited

The contribution by luminous blue variable stars to the dust content of the Magellanic Clouds

C. Agliozzo, N. Phillips, A. Mehner +6

(Shortened) Luminous blue variable stars (LBVs) form dust as a result of episodic, violent mass loss. To investigate their contribution as dust producers in the Magellanic Clouds,…

astro-ph.SR2021★ 55 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.GA2021★ 32 cited

The ASKAP-EMU Early Science Project: 888 MHz Radio Continuum Survey of the Large Magellanic Cloud

Clara M. Pennock, Jacco Th. van Loon, Miroslav D. Filipovic +28

We present an analysis of a new 120 deg radio continuum image of the Large Magellanic Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of $13\rlap{.}^{\prime\…

astro-ph.SR2020★ 20 cited

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…

astro-ph.SR2020★ 32 cited

Evidence for radio and X-ray auroral emissions from the magnetic B-type star rho Oph A

P. Leto, C. Trigilio, F. Leone +20

We present new ATCA multi-wavelength radio measurements (range 2.1-21.2 GHz) of the early-type magnetic star rho Oph A, performed in March 2019 during 3 different observing session…