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Hot Stars in the Galactic Halo

Hot Stars in the Galactic Halo: Proceedings of a Meeting, Held at Union College, Schenectady, New York November 4 6, 1993 in Honor of the 65th Birthda

Hot Stars in the Galactic Halo

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"Hot Stars in the Galactic Halo" by Saul J. Adelman, Arthur R. Upgren, Carol J. Adelman is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

The stars that comprise a halo around our Galaxy are intriguing - they have abundances of elements that suggest they are old. The properties of these 'hot stars' and similar stars in other galaxies challenge the current, well-established theory of stellar evolution in many ways. Studying the collective properties of these stars provides important input to many areas of astrophysics - including the formation of our Galaxy, the late phases of stellar evolution and the stellar populations of other galaxies. The study of hot stars in the halo of our Galaxy is undergoing an exciting renaissance owing to important new observations with the Hubble Space Telescope and ASTRO1 and to techniques recently developed for ground-based observations. Advances in computers have also recently led to a far more detailed and complete theoretical understanding of stellar evolution. A conference was held in Union College, New York, to gather experts in the field and this volume draws together their articles to provide an up-to-date and comprehensive review for graduate students and researchers.

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Best For: Researchers and students interested in stellar evolution and galactic structure
Focus: Properties and elemental abundances of hot stars in the galactic halo
Covers: Analysis of hot stars' characteristics and their implications for stellar evolution theories
Why It Matters: These stars challenge existing stellar evolution models and provide insights into the formation of the Galaxy and late stellar phases

"Hot Stars in the Galactic Halo" by Saul J. Adelman, Arthur R. Upgren, Carol J. Adelman is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Deep Sky & Solar System

Author: Saul J. Adelman, Arthur R. Upgren, Carol J. Adelman

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

The stars that comprise a halo around our Galaxy are intriguing - they have abundances of elements that suggest they are old. The properties of these 'hot stars' and similar stars in other galaxies challenge the current, well-established theory of stellar evolution in many ways. Studying the collective properties of these stars provides important input to many areas of astrophysics - including the formation of our Galaxy, the late phases of stellar evolution and the stellar populations of other galaxies. The study of hot stars in the halo of our Galaxy is undergoing an exciting renaissance owing to important new observations with the Hubble Space Telescope and ASTRO1 and to techniques recently developed for ground-based observations. Advances in computers have also recently led to a far more detailed and complete theoretical understanding of stellar evolution. A conference was held in Union College, New York, to gather experts in the field and this volume draws together their articles to provide an up-to-date and comprehensive review for graduate students and researchers.

AuthorSaul J. Adelman, Arthur R. Upgren, Carol J. Adelman
PublisherCambridge University Press
Published1994-08-25
ISBN-139780521460873
BindingHardcover
Pages246
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System

Format: Hardcover

Length: 246 pages

Language: English

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