activity
20182026
most citedTOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star

51 citations · 112 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

Eating planets makes you younger: The magnetic dynamo rejuvenation of GJ 504 by planetary engulfment

S. Bellotti, C. Pezzotti, G. Buldgen +3

With the discovery of a few thousand exoplanets, questions have been raised regarding star-planet interactions and whether the presence of a companion may affect stellar properties…

astro-ph.SR2026

The attempted polarity reversal and evolving magnetic environment of AD Leo

K. G. Smith, D. Evensberget, S. Bellotti +3

In the past two decades, the observed large-scale magnetic field of the active M dwarf star AD Leo has evolved from strongly to mildly negative, raising a suspicion that it might s…

astro-ph.SR2025

Spectropolarimetric characterisation of exoplanet host stars in preparation of the mission II. The magnetised wind environment of TOI-1860, DS Tuc A, and HD 63433

S. Bellotti, A. Lavail, D. Evensberget +10

We update the status of the spectropolarimetric campaign dedicated to characterise the magnetic field properties of a sample of known exoplanet-hosting stars included in the curren…

astro-ph.SR2024★ 3 cited

Polarization position angle standard stars: a reassessment of and its variability for seventeen stars based on a decade of observations

Daniel V. Cotton, Jeremy Bailey, Lucyna Kedziora-Chudczer +14

Observations of polarization position angle () standards made from 2014 to 2023 with the High Precision Polarimetric Instrument (HIPPI) and other HIPPI-class polarimeters in bot…

astro-ph.SR2024

High-latitude coronal mass ejections on the young solar-like star AB Dor

K. Markus Strickert, Dag Evensberget, Aline A. Vidotto

AB Dor is a young solar-type star with a surface large-scale magnetic field to times stronger than the that of the Sun. Although strong magnetic fields are thought to…

astro-ph.SR2024★ 6 cited

Rotational evolution of young-to-old stars with data-driven three-dimensional wind models

D. Evensberget, A. A. Vidotto

Solar-type stars form with a wide range of rotation rates. A wide range persists until a stellar age of 0.6 Gyr, after which solar-type stars exhibit Skumanich spin-down. Rotationa…

astro-ph.SR2023★ 18 cited

The winds of young Solar-type stars in the Pleiades, AB Doradus, Columba and Pictoris

Dag Evensberget, Stephen C. Marsden, Bradley D. Carter +6

Solar-type stars, which shed angular momentum via magnetised stellar winds, enter the main sequence with a wide range of rotational periods . This initially wide rang…

astro-ph.SR2018★ 18 cited

The Rotationally Modulated Polarization of Boo A

Daniel V. Cotton, Dag Evensberget, Stephen C. Marsden +9

We have observed the active star Boo A (HD 131156A) with high precision broadband linear polarimetry contemporaneously with circular spectropolarimetry. We find both signals ar…