activity
19972026
most citedA change in the optical polarization associated with a gamma-ray flare in the blazar 3C 279

334 citations · 4.5k across the 140 of their papers we have counts for

collaborators
Showing 2017Show all

8 papers · 1 filter

astro-ph.GA2017★ 8 cited

First Extended Catalogue of Galactic Bubbles InfraRed Fluxes from WISE and Herschel Surveys

F. Bufano, P. Leto, D. Carey +8

In this paper, we present the first extended catalogue of far-infrared fluxes of Galactic bubbles. Fluxes were estimated for 1814 bubbles, defined here as the `golden sample', and…

astro-ph.GA2017★ 5 cited

SCORPIO-II: Spectral indices of weak Galactic radio sources

F. Cavallaro, C. Trigilio, G. Umana +10

In the next few years the classification of radio sources observed by the large surveys will be a challenging problem, and spectral index is a powerful tool for addressing it. Here…

astro-ph.GA2017★ 201 cited

Properties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

D. Elia, S. Molinari, E. Schisano +83

Hi-GAL is a large-scale survey of the Galactic plane, performed with Herschel in five infrared continuum bands between 70 and 500 m. We present a band-merged catalogue of spatia…

astro-ph.GA2017★ 36 cited

Spatial distribution of star formation related to ionized regions throughout the inner Galactic plane

P. Palmeirim, A. Zavagno, D. Elia +35

We present a comprehensive statistical analysis of star-forming objects located in the vicinities of 1 360 bubble structures throughout the Galactic Plane and their local environme…

astro-ph.SR2017★ 9 cited

The Luminous Blue Variable RMC127 as seen with ALMA and ATCA

C. Agliozzo, C. Trigilio, G. Pignata +12

We present ALMA and ATCA observations of the luminous blue variable \rmc. The radio maps show for the first time the core of the nebula and evidence that the nebula is strongly asy…

astro-ph.SR2017★ 14 cited

A method to measure the transverse magnetic field and orient the rotational axis of stars

Francesco Leone, Cesare Scalia, Manuele Gangi +5

Direct measurements of the stellar magnetic fields are based on the splitting of spectral lines into polarized Zeeman components. With few exceptions, Zeeman signatures are hidden…