Results 11 to 20 of about 3,640 (192)

Stellar coronal mass ejections – II. Constraints from spectroscopic observations [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT Detections of stellar coronal mass ejections (CMEs) are still rare. Observations of strong Balmer line asymmetries during flare events have been interpreted as being caused by CMEs. Here, we aim to estimate the maximum possible Balmer line fluxes expected from CMEs to infer their detectability in spectroscopic observations ...
Odert, P.   +3 more
openaire   +2 more sources

Detection of a High-velocity Prominence Eruption Leading to a CME Associated with a Superflare on the RS CVn-type Star V1355 Orionis

open access: yesThe Astrophysical Journal, 2023
Stellar coronal mass ejections (CMEs) have recently received much attention for their impacts on exoplanets and stellar evolution. Detecting prominence eruptions, the initial phase of CMEs, as the blueshifted excess component of Balmer lines is a ...
Shun Inoue   +7 more
doaj   +1 more source

Coronal dimming as a proxy for stellar coronal mass ejections [PDF]

open access: yesProceedings of the International Astronomical Union, 2019
AbstractSolar coronal dimmings have been observed extensively in the past two decades and are believed to have close association with coronal mass ejections (CMEs). Recent study found that coronal dimming is the only signature that could differentiate powerful flares that have CMEs from those that do not.
M. Jin   +8 more
openaire   +2 more sources

Tuning the Exospace Weather Radio for Stellar Coronal Mass Ejections [PDF]

open access: yesThe Astrophysical Journal, 2020
Abstract Coronal mass ejections (CMEs) on stars other than the Sun have proven very difficult to detect. One promising pathway lies in the detection of type II radio bursts. Their appearance and distinctive properties are associated with the development of an outward propagating CME-driven shock.
Julián D. Alvarado-Gómez   +9 more
openaire   +2 more sources

Hunting for stellar coronal mass ejections

open access: yes, 2022
Solar flares are often accompanied by filament/prominence eruptions, sometimes leading to coronal mass ejections (CMEs). By analogy, we expect that stellar flares are also associated with stellar CMEs whose properties are essential to know the impact on exoplanet habitability.
Namekata, Kosuke   +5 more
openaire   +2 more sources

A stellar flare−coronal mass ejection event revealed by X-ray plasma motions [PDF]

open access: yesNature Astronomy, 2019
Letter published on Nature Astronomy, see https://rdcu.be ...
C. Argiroffi   +8 more
openaire   +5 more sources

Stellar coronal mass ejections – I. Estimating occurrence frequencies and mass-loss rates [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
18 pages, 8 figures, 1 table, accepted to ...
Odert, P.   +3 more
openaire   +2 more sources

Full Velocities and Propagation Directions of Coronal Mass Ejections Inferred from Simultaneous Full-disk Imaging and Sun-as-a-star Spectroscopic Observations

open access: yesThe Astrophysical Journal, 2023
Coronal mass ejections (CMEs) are violent ejections of magnetized plasma from the Sun that can trigger geomagnetic storms, endanger satellite operations, and destroy electrical infrastructures on the Earth.
Hong-peng Lu   +8 more
doaj   +1 more source

First detections of stellar coronal mass ejections through coronal dimmings [PDF]

open access: yes, 2020
Abstract The authors have requested that this preprint be removed from Research Square.
Astrid Veronig   +5 more
openaire   +1 more source

Detection of Coronal Mass Ejections in V471 Tauri with the Hubble Space Telescope [PDF]

open access: yes, 2001
V471 Tauri, an eclipsing system consisting of a hot DA white dwarf (WD) and a dK2 companion in a 12.5-hour orbit, is the prototype of the pre-cataclysmic binaries.
Arnaud M.   +8 more
core   +2 more sources

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