activity
20182025
most citedSlingshot prominences: coronal structure, mass loss and spin down

23 citations · 28 across the 4 of their papers we have counts for

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10 papers · 1 filter

astro-ph.SR2025★ 1 cited

Far beyond the Sun: III. The magnetic cycle of Horologii

Julián D. Alvarado-Gómez, Gaitee A. J. Hussain, Eliana M. Amazo-Gómez +6

We present a comprehensive investigation of the magnetic cycle of the young, active solar analogue Horologii ( Hor) based on intensive spectropolarimetric monitoring using H…

astro-ph.SR2025★ 4 cited

Short- and long-term variations of the high mass accretion rate classical T Tauri star DR Tau

Gabriella Zsidi, Ágnes Kóspál, Péter Ábrahám +20

Classical T Tauri stars are newly formed, low mass stars which may display both periodic and random variations in their brightness. The interaction between the star and its circums…

astro-ph.SR2023

First Chromospheric Activity and Doppler Imaging Study of PW And Using a New Doppler Imaging Code: SpotDIPy

Engin Bahar, Hakan V. Şenavcı, Emre Işık +4

Measuring coverage of dark spots on cool stars is important in understanding how stellar magnetic activity scales with the rotation rate and convection zone depth. In this respect,…

astro-ph.SR2021

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…

astro-ph.SR2020

Identifying solar-like magnetic cycles with Zeeman-Doppler-Imaging (ZDI)

Lisa T. Lehmann, Gaitee A. J. Hussain, Aline A. Vidotto +2

We are reaching the point where spectropolarimetric surveys have run for long enough to reveal solar-like magnetic activity cycles. In this paper we investigate what would be the b…

astro-ph.SR2019★ 23 cited

Slingshot prominences: coronal structure, mass loss and spin down

M. Jardine, A. Collier Cameron, J. -F. Donati +1

The structure of a star's coronal magnetic field is a fundamental property that governs the high-energy emission from the hot coronal gas and the loss of mass and angular momentum…