activity
20142023
most citedNew PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star forming dwarf galaxies

496 citations · 653 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2023★ 3 cited

Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?

Daniele Telloni, Gary P. Zank, Laxman Adhikari +32

Evidence for the presence of ion cyclotron waves, driven by turbulence, at the boundaries of the current sheet is reported in this paper. By exploiting the full potential of the jo…

astro-ph.IM2022★ 4 cited

From Assembly to the Complete Integration and Verification of the SOXS Common Path

Kalyan Kumar Radhakrishnan Santhakumari, Federico Battaini, Riccardo Claudi +50

The Son Of X-Shooter (SOXS) is a single object spectrograph offering simultaneous spectral coverage in UV-VIS (350-850 nm) and NIR (800-2000 nm) wavelength regimes with an average…

astro-ph.IM2022

Laboratory test of the VIS detector system of SOXS for the ESO-NTT telescope

Rosario Cosentino, Marcos Hernandez, Hector Ventura +45

SOXS is the new spectrograph for the ESO NTT telescope able to cover the optical and NIR bands thanks to two different arms: the UV-VIS (350-850 nm), and the NIR (800-2000 nm). In…

astro-ph.SR2022★ 18 cited

A Coronal Mass Ejection followed by a prominence eruption and a plasma blob as observed by Solar Orbiter

A. Bemporad, V. Andretta, R. Susino +26

On February 12, 2021 two subsequent eruptions occurred above the West limb, as seen along the Sun-Earth line. The first event was a typical slow Coronal Mass Ejection (CME), follow…

astro-ph.SR2021★ 50 cited

First light observations of the solar wind in the outer corona with the Metis coronagraph

M. Romoli, E. Antonucci, V. Andretta +65

The investigation of the wind in the solar corona initiated with the observations of the resonantly scattered UV emission of the coronal plasma obtained with UVCS-SOHO, designed to…

astro-ph.GA2021★ 25 cited

On the effects of the Initial Mass Function on Galactic chemical enrichment

S. Goswami, A. Slemer, P. Marigo +7

There is mounting evidence that the stellar initial mass function (IMF) could extend much beyond the canonical Mi ~100, Msun limit, but the impact of such hypothesis on the chemica…

astro-ph.IM2021★ 10 cited

Cosmic-ray flux predictions and observations for and with Metis on board Solar Orbiter

C. Grimani, V. Andretta, P. Chioetto +41

The Metis coronagraph is one of the remote sensing instruments hosted on board the ESA/NASA Solar Orbiter mission. Metis is devoted to carry out the first simultaneous imaging of t…

astro-ph.GA2017★ 2 cited

Modelling the UV to radio SEDs of nearby star-forming galaxies: new Parsec SSP for Grasil

I. A. Obi, A. Bressan, F. Perrotta +9

By means of the updated PARSEC database of evolutionary tracks of massive stars, we compute the integrated stellar light, the ionizing photon budget and the supernova rates of youn…

astro-ph.SR2015★ 10 cited

Envelope Overshooting in Low Metallicity Intermediate- and High-mass Stars: a test with the Sagittarius Dwarf Irregular Galaxy

Jing Tang, Alessandro Bressan, Alessandra Slemer +5

We check the performance of the {\sl\,PARSEC} tracks in reproducing the blue loops of intermediate age and young stellar populations at very low metallicity. We compute new evoluti…

nucl-ex2015★ 35 cited

Strengths of the resonances at 436, 479, 639, 661, and 1279 keV in the Ne(p,)Na reaction

Rosanna Depalo, Francesca Cavanna, Federico Ferraro +11

The Ne(p,)Na reaction is included in the neon-sodium cycle of hydrogen burning. A number of narrow resonances in the Gamow window dominates the thermonuclear react…

astro-ph.SR2014★ 496 cited

New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star forming dwarf galaxies

Jing Tang, Alessandro Bressan, Philip Rosenfield +4

We extend the {\sl\,PARSEC} library of stellar evolutionary tracks by computing new models of massive stars, from 14\Msun to 350\Msun. The input physics is the same used in the {\s…