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

We have investigated the X-ray emission from the shock-heated plasma of the Galactic supernova remnant Kesteven 69 with\udXMM-Newton. Assuming the plasma is at collisional ionization equilibrium, a plasma temperature and a column absorption\udare found to be kT ~ 0.62 keV and NH ~ 2.85 ×1022 cm-2 respectively by imaging spectroscopy. Together with the deduced\udemission measure, we place constraints on its Sedov parameters

Exploring the Diffuse X-ray Emission of Supernova Remnant Kesteven 69 with XMM-Newton