REVIEW
X-ray variability of cool stars: Magnetic activity and accretion
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
X-ray variability of cool stars: Magnetic activity and accretion
classification
astro-ph.SR
keywords
starsvariabilityx-rayaccretionachievementsactivityarticlecool
read the original abstract
This article provides a review of X-ray variability from late-type stars with particular focus on the achievements of XMM-Newton and its potential for future studies in this field.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.