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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Coronae exist in most astrophysical objects: stars, accretion disks, andindividual galaxies and clusters of galaxies. Coronae in these varied systemshave some common properties: 1) hydrostatic equilibrium in background gravityis a good assumption; 2) they are optically thin, i.e., photons escape as soonas they are born; 3) they have cooling times shorter than their ages, and thusrequire heating for sustenance. Generally the coronal heating mechanisms arequite complex but the structure of the corona is tightly constrained by theinterplay of cooling, {\em global} heating, and background gravity. We brieflysummarize the results from our studies of the intracluster medium (the clustercorona) and draw inferences which should apply to most astrophysical coronae.

Astrophysical Coronae: Lessons from Modeling of the Intracluster Medium