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Luminous Stars in Nearby Galaxies
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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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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 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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Origin and Evolution of the Elements
of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains;
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Origin and Evolution of the Elements
of stars in different locations within our Galaxy and nearby galaxies is discussed, as are the compositions of hot and cold gases, of dust grains;
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Become One
About the CoverThe image on the cover (NGC 6240) is a well-studied nearby ultra luminous infrared galaxy in the constellation Ophiuchus;
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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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Dwarf Galaxies (IAU S344)
Dwarf galaxies are important tools for understanding structure formation and galaxy evolution across cosmic time. These low-mass systems;
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Massive Stars As Cosmic Engines (Iau S250)
explosions which enrich galaxies in elements such as oxygen, and sometimes their demise is associated with intense bursts of gamma-rays. IAU;
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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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Black Holes from the Stars to Galaxies--Across the Range of Masses
holes in binary stellar systems; and, possibly, of intermediate-mass black holes in ultraluminous X-ray sources in nearby galaxies. Black holes;
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The Magellanic System
processes within them. Observations of these nearby dwarf galaxies continue to advance, calibrate and challenge our knowledge of the cosmos. They;
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Cambridge Contemporary Astrophysics
stellar nucleosynthesis, abundance determinations in stars and ionised nebulae, chemical composition of nearby and distant galaxies, and models;
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Cosmochemistry
stellar nucleosynthesis, abundance determinations in stars and ionised nebulae, chemical composition of nearby and distant galaxies, and models;
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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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Astroquizzical: Solving the Cosmic Puzzles of Our Planets, Stars, and Galaxies
Exploring the family tree of the cosmos, from humans on Earth to stars and galaxies to the first atoms of the Big Bang; with striking;
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Why Galaxies Care about AGB Stars (IAU S343)
populations and the chemical evolution of galaxies. Our understanding of these complex stars is given using insights into many aspects of physics and;
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Stars and Galaxies
With this newly revised Ninth Edition of STARS AND GALAXIES, the authors' goals are to help you use astronomy to understand science--and;
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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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Galaxies at High Redshift
studies based on far-infrared diagnostics, it reviews quasar absorption lines, and the properties of nearby galaxies. Each chapter is written by a;
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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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Galactic Dynamics in the Era of Large Surveys (IAU S353)
Galactic dynamics is fundamental to understanding the formation of galaxies, their internal evolution and their current structure. While;
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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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Galaxies at High Redshift
studies based on far-infrared diagnostics, it reviews quasar absorption lines, and the properties of nearby galaxies. Each chapter is written by a;
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