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From Dust to Stars [electronic resource] :Studies of the Formation and Early Evolution of Stars / by Norbert S. Schulz.

by Schulz, Norbert S [author.]; SpringerLink (Online service).
Material type: materialTypeLabelBookSeries: Springer Praxis Books, Astronomy and Planetary Sciences: Publisher: Berlin, Heidelberg : Springer Berlin Heidelberg, 2005.Description: XVI, 390 p. online resource.ISBN: 9783540273219.Subject(s): Physics | Physical geography | Astronomy | Astrophysics | Physics | Astrophysics | Astronomy | Extraterrestrial Physics, Space Sciences | Geophysics/GeodesyDDC classification: 523.01 Online resources: Click here to access online
Contents:
About the Book -- Historical Background -- Studies of Interstellar Matter -- Molecular Clouds and Cores -- Concepts of Stellar Collapse -- Evolution of Young Stellar Objects -- Accretion Phenomena and Magnetic Activity in YSOs -- High-energy Signatures in YSOs -- Star-forming Regions -- Proto-solar Systems and the Sun.
In: Springer eBooksSummary: Studies of stellar formation in galaxies have a profound impact on our understanding of the present and the early universe. The book describes complex physical processes involved in the creation of stars and during their young lives. It illustrates how these processes reveal themselves from radio wavelengths to high energy X-rays and gamma -rays, with special reference towards high energy signatures. Several sections devoted to key analysis techniques demonstrate how modern research in this field is pursued.
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QB460-466 (Browse shelf) Available

About the Book -- Historical Background -- Studies of Interstellar Matter -- Molecular Clouds and Cores -- Concepts of Stellar Collapse -- Evolution of Young Stellar Objects -- Accretion Phenomena and Magnetic Activity in YSOs -- High-energy Signatures in YSOs -- Star-forming Regions -- Proto-solar Systems and the Sun.

Studies of stellar formation in galaxies have a profound impact on our understanding of the present and the early universe. The book describes complex physical processes involved in the creation of stars and during their young lives. It illustrates how these processes reveal themselves from radio wavelengths to high energy X-rays and gamma -rays, with special reference towards high energy signatures. Several sections devoted to key analysis techniques demonstrate how modern research in this field is pursued.

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