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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

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Showing astro-ph.SRShow all

5 papers · 1 filter

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.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.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…

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…