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The Stellar Populations of Galaxies

; secondly from nearby galaxies where stars can still be resolved; and thirdly in remote galaxies in which the stellar population can only be studied;

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Evolution of Stars and Stellar Populations

study of stellar populations in galaxies. Taking a unique approach to the subject, this self contained text introduces first the theory;

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Star Clusters (IAU S351)

articles on the build up of larger galaxies from smaller galaxies and stellar clusters, and discussions of the latest data from large surveys and;

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Cambridge Contemporary Astrophysics

on the meeting, reviewing how the study of stars in nearby galaxies can be used to understand stellar and galactic structure and evolution;

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Cambridge Contemporary Astrophysics

on the meeting, reviewing how the study of stars in nearby galaxies can be used to understand stellar and galactic structure and evolution;

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Why Galaxies Care about AGB Stars (IAU S343)

different time scales. IAU Symposium 343 builds a bridge between research on AGB stars themselves and their applications to the modelling of stellar;

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The Properties of Star-Forming Galaxies at z~2

We study the properties of star-forming galaxies at redshift z 2, an era in which a substantial fraction of the stellar mass in the;

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Hot Stars in the Galactic Halo

of these 'hot stars' and similar stars in other galaxies challenge the well-established theory of stellar evolution in many ways. Studying the;

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Galaxy Masses As Constraints of Formation Models

advance in recent years has been the enrichment of studies of the luminosity evolution of galaxies with determinations of their stellar or total;

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Galaxy Formation and Evolution

growth of cosmic structure; processes affecting the gaseous and dark matter components of galaxies and their stellar populations; the formation;

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The Intriguing Life of Massive Galaxies (Iau S295)

The lives of massive galaxies are affected by many key processes, including gas accretion and star formation, feedback and quenching, black;

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Formation and Evolution of Galaxy Outskirts (IAU S321)

The borders between galaxies and the almost empty intergalactic medium are ill-defined regions where gas struggles to form stars. The;

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Black Holes from the Stars to Galaxies--Across the Range of Masses

overwhelming evidence in favour of the presence of supermassive black holes at the centre of galaxies, including the Milky Way; of stellar-mass black;

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Galaxies In 3D Across The Universe IAU S

IAU Symposium 309 contains contributions on the timely theme of spatially and energetically resolved properties of galaxies. New;

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Galactic Dynamics in the Era of Large Surveys (IAU S353)

galactic dynamics has traditionally focused on the evolution of the stellar components of galaxies, studies over the past two decades have shown;

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Dynamics of Galaxies

Our understanding of galaxies, the building blocks of the Universe has advanced significantly in recent years. New observations from ground;

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Proceedings of the International Astronomical Union Symposia and Colloquia

observations, from stars and stellar orbits through nearby black holes and explosive events, to the building blocks and transport of energy in galaxies;

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Instability, Chaos and Predictability in Celestial Mechanics and Stellar Dynamics

sections: chaos, ergodic and stochastic motion, stellar systems and galaxies, triple and many body problem, and general celestial mechanics and;

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From Luminous Hot Stars to Starburst Galaxies

Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their;

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RR Lyrae Stars

, both in the Milky Way and other galaxies, and as an outstanding testing ground for stellar evolution and pulsation theories. He stresses the;

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Cambridge Contemporary Astrophysics

in the study of planet formation and the late chemical evolution of galaxies. This book covers many aspects, from spectral line formation to;

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Galactic Dynamics

astrophysicists, use the tools of theoretical physics to describe how galaxies and other stellar systems work, succinctly and lucidly explaining;

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Proceedings of the International Astronomical Union Symposia and Colloquia

and loss, and magnetic fields; and they help trace stellar populations, the kinematics, and chemistry of galaxies including our own galaxy;

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The Metal-Rich Universe

in the study of planet formation and the late chemical evolution of galaxies. This book covers many aspects, from spectral line formation to;

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Cambridge Astrophysics

Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their;

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The Nearest Active Galaxies

Reprinted from Astrophysics and Space Science vol. 205, no. 1 (1993), over 30 articles discuss aspects of some nearby galaxies. The topics;

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Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28

Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma rays;

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