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Evolution of Stars and Stellar Populations

Evolution of Stars and Stellar Populations is a comprehensive presentation of the theory of stellar evolution and its application to the;

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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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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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Cambridge Contemporary Astrophysics

stellar formation and evolution in high metallicity regimes. It is invaluable to researchers and graduate students in stellar evolution;

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The Metal-Rich Universe

stellar formation and evolution in high metallicity regimes. It is invaluable to researchers and graduate students in stellar evolution;

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The Art of Modeling Stars in the 21st Century (Iau S252)

recent advances in modelling of stellar structure and evolution. Modelling of stars relies on our understanding of the detailed physical;

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An Introduction to Stellar Astrophysics

, computer simulations and modeling of stars and their evolution. An Introduction to Stellar Astrophysics is a concise textbook containing core;

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An Introduction to Stellar Astrophysics

, computer simulations and modeling of stars and their evolution. An Introduction to Stellar Astrophysics is a concise textbook containing core;

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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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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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Magnetic Fields Throughout Stellar Evolution

All phases of stellar evolution are influenced by the presence of magnetic fields in the star's interior and close environment. IAU;

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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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Cambridge Astrophysics

Like the Earth and planets, stars rotate. Understanding how stars rotate is central to modelling their structure, formation and evolution;

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Cambridge Astrophysics

Like the Earth and planets, stars rotate. Understanding how stars rotate is central to modelling their structure, formation and evolution;

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From Luminous Hot Stars to Starburst Galaxies

lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and;

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Cambridge Astrophysics

lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and;

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Galaxy Masses As Constraints of Formation Models

measure the masses of stars, gas and dark matter in galaxies, and explores what these mass determinations tell us about galaxy evolution. A key;

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The Ages of Stars

Estimating accurate stellar ages is one of the most difficult challenges in astrophysics. A star's age cannot be measured directly, and;

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Introduction to Stellar Astrophysics

structure, evolution, and observed properties of stars. The first half of the book explains how stellar motions, distances, luminosities, colours;

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Stellar Evolution Physics 2 Volume Hardback Set Stellar Evolution Physics

the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to;

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Dust and Molecules in Evolved Stars

evolved stars. This book brings together the leading astronomers and astrophysicists in the field of molecular astrophysics and stellar physics;

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Dust and Molecules in Evolved Stars

evolved stars. This book brings together the leading astronomers and astrophysicists in the field of molecular astrophysics and stellar physics;

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Young Stars Planets Near Sun IAU S314

, these stars provide unique opportunities to investigate early stellar evolution, and they offer readily accessible targets for direct imaging;

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Stars and Stellar Processes

processes and energy transport in stellar interiors, and stellar evolution from star formation to the common stellar endpoints as white dwarfs and;

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Stellar Astrophysical Fluid Dynamics

of knowledge in stellar astrophysical fluid dynamics, and its publication marked the 60th birthday of Douglas Gough, Professor of Theoretical Physics;

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Formation and Evolution of Galaxy Outskirts (IAU S321)

astronomical instruments. They discuss the most recent advances in the study of the stellar, dust and gas content of galaxy outskirts, going from;

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