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 Tools annual

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 monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

As we strive to understand how galaxies evolve it is crucial that we resolvephysical processes and test emerging theories in nearby systems that we canobserve in great detail. Our own Galaxy, the Milky Way, and the nearbyMagellanic Clouds provide unique windows into the evolution of galaxies, eachwith its own metallicity and star formation rate. These laboratories allow usto study with more detail than anywhere else in the Universe how galaxiesacquire fresh gas to fuel their continuing star formation, how they exchangegas with the surrounding intergalactic medium, and turn warm, diffuse gas intomolecular clouds and ultimately stars. The $\lambda$21-cm line of atomichydrogen (HI) is an excellent tracer of these physical processes. With the SKAwe will finally have the combination of surface brightness sensitivity, pointsource sensitivity and angular resolution to transform our understanding of theevolution of gas in the Milky Way, all the way from the halo down to theformation of individual molecular clouds.

Galactic and Magellanic Evolution with the SKA