English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

The measurement of stellar properties such as chemical compositions, massesand ages, through stellar spectra, is a fundamental problem in astrophysics.Progress in the understanding, calculation and measurement of atomic propertiesand processes relevant to the high-accuracy analysis of F-, G-, and K-typestellar spectra is reviewed, with particular emphasis on abundance analysis.This includes fundamental atomic data such as energy levels, wavelengths, andtransition probabilities, as well as processes of photoionisation, collisionalbroadening and inelastic collisions. A recurring theme throughout the review isthe interplay between theoretical atomic physics, laboratory measurements, andastrophysical modelling, all of which contribute to our understanding of atomsand atomic processes, as well as to modelling stellar spectra.

Accurate abundance analysis of late-type stars: advances in atomic physics