Titlebook: Lessons from the Local Group; A Conference in hono Kenneth Freeman,Bruce Elmegreen,Matthew Woolway Conference proceedings 2015 Springer Int

Coterminous

Cloud and Star Formation in Spiral Arms,onal instabilities, arguing that the former is prevalent at lower galactic surface densities and the latter at higher. Cloud masses are also limited by stellar feedback, which can be effective before clouds reach their maximum mass. We show other properties of clouds in simulations with different le

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CANON

Urologist

Gas and Star Formation in M33: An Artistic Pathway,high resolution data to shed light on its assembly and star formation across cosmic time. I will summarize some of the key ingredients related to the formation and evolution of this galaxy, such as its dark matter, the baryonic distribution and the metallicity gradients. M33 is a pure disk galaxy wi

Schlemms-Canal

Depicting the Early Evolution of Globular Clusters Through the Lens of Multiple Stellar Populationsout of homogeneous material. Indeed, detailed spectroscopic studies of GC long-lived low-mass stars performed with 8–10 m class telescopes, together with high-precision photometry of Galactic GCs obtained with HST, have brought compelling evidences on the presence of multiple stellar populations in

Oration

Globular Clusters and Two Phase Galaxy Formation: The Milky Way and Beyond,ty maps for 25 nearby early type galaxies out to, typically, 2-3 . for galaxy starlight, and 8-10 . for globular clusters. While other surveys have much larger galaxy samples, the SLUGGS “claim to fame” is its unprecedentedly wide field coverage coupled with exquisite velocity resolution (∼12 km s.)

箴言

Globular Clusters in the Local Group,assembly. Those hosted by galaxies in the Local Group play a key role in this work, as they may be studied in great detail on a star-by-star basis along with the surrounding field populations. In this contribution I describe how new results from the PAndAS survey are revolutionising our view of the

Concrete

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