activity
20102026
most citedThe active lives of stars: a complete description of rotation and XUV evolution of F, G, K, and M dwarfs

253 citations · 2.9k across the 51 of their papers we have counts for

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16 papers · 1 filter

astro-ph.SR2020★ 253 cited

The active lives of stars: a complete description of rotation and XUV evolution of F, G, K, and M dwarfs

Colin P. Johnstone, Michael Bartel, Manuel Güdel

Aims. We study the evolution of rotation and high energy X-ray, extreme ultraviolet (EUV), and Ly-alpha emission for F, G, K, and M dwarfs, with masses between 0.1 and 1.2 Msun, an…

astro-ph.SR2020★ 31 cited

The solar wind from a stellar perspective: how do low-resolution data impact the determination of wind properties?

S. Boro Saikia, M. Jin, C. P. Johnstone +5

Alfvén-wave-driven 3D magnetohydrodynamic (MHD) models, which are increasingly used to predict stellar wind properties, contain unconstrained parameters and rely on low-resolution…

astro-ph.SR2019★ 10 cited

Stellar activity and planetary atmosphere evolution in tight binary star systems

C. P. Johnstone, E. Pilat-Lohinger, T. Lüftinger +2

Context. In tight binary star systems, tidal interactions can significantly influence the rotational and orbital evolution of both stars, and therefore their activity evolution. Th…

astro-ph.SR2019★ 16 cited

Slingshot prominence evolution for a solar-like star

Carolina Villarreal D'Angelo, Moira Jardine, Colin P. Johnstone +1

Although the present-day Sun rotates too slowly to exhibit centrifugally-supported 'slingshot prominences', at some time during its past it may have formed these clouds of cool gas…

astro-ph.SR2016★ 72 cited

Identifying the "true" radius of the hot sub-Neptune CoRoT-24b by mass loss modelling

H. Lammer, N. V. Erkaev, L. Fossati +8

For the hot exoplanets CoRoT-24b and CoRoT-24c, observations have provided transit radii R of 3.70.4 R and 4.90.5 R, and masses of 5.…

astro-ph.SR2015

Stellar magnetic activity and their influence on the habitability of exoplanets

T. Lüftinger, M. Güdel, C. P. Johnstone

Stellar magnetism, explorable via polarimetry, is a crucial driver of activity, ionization, photodissociation, chemistry and winds in stellar environments. Thus it has an important…

astro-ph.SR2015★ 37 cited

Short-period stellar activity cycles with Kepler photometry

Oleksiy V. Arkhypov, Maxim L. Khodachenko, Helmut Lammer +3

We study the short-periodic component of stellar activity with a cycle periods Pcyc up to 1000 days using the Kepler mission photometry of fast-rotating (rotational periods from 1…

astro-ph.SR2015

The Coronal Temperatures of Low-Mass Main-Sequence Stars

Colin P. Johnstone, Manuel Güdel

Aims. We study the X-ray emission of low-mass main-sequence stars to derive a reliable general scaling law between coronal temperature and the level of X-ray activity. Methods. We…

astro-ph.SR2015★ 251 cited

The Extreme Ultraviolet and X-Ray Sun in Time: High-Energy Evolutionary Tracks of a Solar-Like Star

Lin Tu, Colin P. Johnstone, Manuel Güdel +1

Aims. We aim to describe the pre-main sequence and main-sequence evolution of X-ray and extreme-ultaviolet radiation of a solar mass star based on its rotational evolution starting…

astro-ph.SR2015★ 107 cited

Stellar Winds on the Main-Sequence I: Wind Model

C. P. Johnstone, M. Güdel, T. Lüftinger +2

Aims: We develop a method for estimating the properties of stellar winds for low-mass main-sequence stars between masses of 0.4 and 1.1 solar masses at a range of distances from th…

astro-ph.SR2015★ 229 cited

Stellar Winds on the Main-Sequence II: the Evolution of Rotation and Winds

C. P. Johnstone, M. Güdel, I. Brott +1

Aims: We study the evolution of stellar rotation and wind properties for low-mass main-sequence stars. Our aim is to use rotational evolution models to constrain the mass loss rate…

astro-ph.SR2015★ 14 cited

Colliding Winds in Low-Mass Binary Star Systems: wind interactions and implications for habitable planets

C. P. Johnstone, A. Zhilkin, E. Pilat-Lohinger +3

Context. In binary star systems, the winds from the two components impact each other, leading to strong shocks and regions of enhanced density and temperature. Potentially habitabl…

astro-ph.SR2013

Constraining Stellar Winds of Young Sun-like Stars

Colin P. Johnstone, Theresa Lüftinger, Manuel Güdel +1

As part of the project Pathways to Habitability (http://path.univie.ac.at/), we study the properties of the stellar winds of low-mass and Sun-like stars, and their influences on th…

astro-ph.SR2012

Splinter Session "Solar and Stellar Flares"

L. Fletcher, H. S. Hudson, G. Cauzzi +8

This summary reports on papers presented at the Cool Stars-16 meeting in the splinter session "Solar and Stellar flares." Although many topics were discussed, the main themes were…

astro-ph.SR2010★ 28 cited

The contribution of starspots to coronal structure

Doris Arzoumanian, Moira Jardine, Jean-François Donati +2

Significant progress has been made recently in our understanding of the structure of stellar magnetic fields, thanks to advances in detection methods such as Zeeman-Doppler Imaging…

astro-ph.SR2010★ 27 cited

Modelling stellar coronae from surface magnetograms: the role of missing magnetic flux

Colin Johnstone, Moira Jardine, Duncan Mackay

Recent advances in spectropolarimetry have allowed the reconstruction of stellar coronal magnetic fields. This uses Zeeman-Doppler magnetograms of the surface magnetic field as a l…