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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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From Interstellar Clouds to Star-Forming Galaxies (IAU S315)

the first star-forming galaxies at high redshift, it makes connections between the latest observations and advanced numerical simulations. It;

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The Physics and Evolution of Active Galactic Nuclei

them and other astronomical objects. Recent developments regarding the evolutionary connections between active galaxies and star-forming;

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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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Environment and the Formation of Galaxies: 30 years later

at z 1 and the implementation of environmental effects in cosmological models of galaxy formation and evolution. This book presents the;

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Dwarf Galaxies (IAU S344)

, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and;

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The Magellanic System

fields of research discuss galactic dynamics, the physics of the interstellar medium and star formation, and the fundamental properties and;

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Starburst Galaxies

located towards the centers of host galaxies. Studies of this kind of star formation at high redshift have produced astonishing results;

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Mass-Transfer Induced Activity in Galaxies

large-scale properties of the host galaxy. The crucial question is what triggers and fuels nuclear activity now and at earlier epochs? The;

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Evolution of Stars and Stellar Populations

population and describes stellar population synthesis methods to study ages and star formation histories of star clusters and galaxies. The book;

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Galaxies at High Redshift

methods suited to the study of distant galaxies. This volume contains the lectures delivered at the XI Canary Islands Winter School;

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Studying Distant Galaxies: A Handbook Of Methods And Analyses

. It also paves the way for establishing relations between fundamental properties of distant galaxies. At each step, the reader is assisted;

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Studying Distant Galaxies: A Handbook Of Methods And Analyses

. It also paves the way for establishing relations between fundamental properties of distant galaxies. At each step, the reader is assisted;

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Galaxies at High Redshift

methods suited to the study of distant galaxies. This volume contains the lectures delivered at the XI Canary Islands Winter School;

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Stars and galaxies

into deep space to look at the billions of stars and galaxies that make up our universe. Starting with our own star, the Sun, we examine what;

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Cambridge Astrophysics

Globular clusters are roughly spherical, densely packed groups of stars found around galaxies. Most globular clusters probably formed at;

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Space at the Speed of Light

An astrophysicist at the University of Oxford and popular YouTube star offers ten accessible and engaging lessons covering everything you;

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Astronomy Physical Perspective

stars, galaxies and the solar system. The text looks at the properties of stars, star formation and evolution; neutron stars and black holes;

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Astrophysics of the Interstellar Medium

Cosmology at Padova University. From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds;

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Astrophysics of the Interstellar Medium

Cosmology at Padova University. From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds;

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Low-Metallicity Star Formation (Iau S255)

dwarf galaxies, because they are metal poor and because of their kinematics and structure, can tell us about how star formation proceeded in the;

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Near-Field Cosmology with Dwarf Elliptical Galaxies

Dwarf galaxies offer a valuable insight into the physical processes that govern galaxy formation and evolution at high redshift. These;

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Molecular Gas, Dust, And Star Formation In Galaxies (Iau S29

Our knowledge of the molecular gas content in galaxies has advanced rapidly in the past decade with systematic surveys from ground-based;

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Galaxies and Other Deep-Sky Objects

-to-use field guide covering more than 70 deep-sky objects; a complete overview of the evolution of galaxies, nebulae, quasars, star clusters;

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Galactic Astronomy

simpler to understand. Binney and Merrifield introduce all astronomical concepts necessary to understand the properties of galaxies, including;

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The Sun as a Star

, Galaxies and The Stars, Roger Tayler presents the first full picture of how studies of the Sun and the solar system help us understand stars;

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Nuclear Activity in Galaxies Across Cosmic Time (IAU S356)

IAU Symposium 356 summarises the most recent results in the field of active galaxies and active galactic nuclei (AGN). These are some;

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