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The Physics of Star Formation and Early Stellar Evolution (1991)

The Physics of Star Formation and Early Stellar Evolution

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"The Physics of Star Formation and Early Stellar Evolution" by Charles J. Lada, N.D. Kylafis is a astronomy book and space science reference focused on Deep Sky & Solar System. Best for students, researchers, and serious astronomy enthusiasts.

Proceedings of the NATO Advanced Study Institute, Agia Pelagia, Crete, Greece, May 27-June 8, 1990

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Best For: Researchers and graduate students in astrophysics focusing on star formation and early stellar evolution.
Focus: Detailed proceedings from a 1990 NATO Advanced Study Institute covering the physics behind star formation and the initial stages of stellar development.
Covers: Theoretical and observational studies presented during the institute, including mechanisms of star formation and early stellar processes.
Why It Matters: Provides foundational insights and research findings from a specialized scientific meeting, useful for understanding the physical processes in early stellar evolution.

"The Physics of Star Formation and Early Stellar Evolution" by Charles J. Lada, N.D. Kylafis 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: Charles J. Lada, N.D. Kylafis

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.

Proceedings of the NATO Advanced Study Institute, Agia Pelagia, Crete, Greece, May 27-June 8, 1990

AuthorCharles J. Lada, N.D. Kylafis
PublisherSpringer
Published1991-07-31
ISBN-139780792313496
BindingHardcover
Pages794
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesNATO Science Series C:

Format: Hardcover

Length: 794 pages

Language: English

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