Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237)

Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237) PDF Author: International Astronomical Union. Symposium
Publisher: Cambridge University Press
ISBN: 9780521863469
Category : Science
Languages : en
Pages : 544

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Book Description
New stars form in the dense turbulent gas clouds of galaxies, and the formation of these clouds is the subject of the IAU S237. This book is the most up-to-date review of all aspects of cloud and star formation, and one of the few compendiums available on ISM turbulence.

Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237)

Triggered Star Formation in a Turbulent Interstellar Medium (IAU S237) PDF Author: International Astronomical Union. Symposium
Publisher: Cambridge University Press
ISBN: 9780521863469
Category : Science
Languages : en
Pages : 544

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Book Description
New stars form in the dense turbulent gas clouds of galaxies, and the formation of these clouds is the subject of the IAU S237. This book is the most up-to-date review of all aspects of cloud and star formation, and one of the few compendiums available on ISM turbulence.

Triggered Star Formation in a Turbulent ISM

Triggered Star Formation in a Turbulent ISM PDF Author: International Astronomical Union. Symposium
Publisher:
ISBN:
Category : Interstellar matter
Languages : en
Pages :

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Book Description


Star Formation Efficiency in the Turbulent, Interstellar Medium (ISM)

Star Formation Efficiency in the Turbulent, Interstellar Medium (ISM) PDF Author: Manuel Oliver Stubbe
Publisher:
ISBN:
Category :
Languages : en
Pages :

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Book Description


Physics of the Interstellar and Intergalactic Medium

Physics of the Interstellar and Intergalactic Medium PDF Author: Bruce T. Draine
Publisher: Princeton University Press
ISBN: 1400839084
Category : Science
Languages : en
Pages : 560

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Book Description
This is a comprehensive and richly illustrated textbook on the astrophysics of the interstellar and intergalactic medium--the gas and dust, as well as the electromagnetic radiation, cosmic rays, and magnetic and gravitational fields, present between the stars in a galaxy and also between galaxies themselves. Topics include radiative processes across the electromagnetic spectrum; radiative transfer; ionization; heating and cooling; astrochemistry; interstellar dust; fluid dynamics, including ionization fronts and shock waves; cosmic rays; distribution and evolution of the interstellar medium; and star formation. While it is assumed that the reader has a background in undergraduate-level physics, including some prior exposure to atomic and molecular physics, statistical mechanics, and electromagnetism, the first six chapters of the book include a review of the basic physics that is used in later chapters. This graduate-level textbook includes references for further reading, and serves as an invaluable resource for working astrophysicists. Essential textbook on the physics of the interstellar and intergalactic medium Based on a course taught by the author for more than twenty years at Princeton University Covers radiative processes, fluid dynamics, cosmic rays, astrochemistry, interstellar dust, and more Discusses the physical state and distribution of the ionized, atomic, and molecular phases of the interstellar medium Reviews diagnostics using emission and absorption lines Features color illustrations and detailed reference materials in appendices Instructor's manual with problems and solutions (available only to teachers)

The Dense Interstellar Medium in Galaxies

The Dense Interstellar Medium in Galaxies PDF Author: Susanne Pfalzner
Publisher: Springer Science & Business Media
ISBN: 3642189024
Category : Science
Languages : en
Pages : 665

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Book Description
The Cologne-Bonn-Zermatt symposium is a well established series of conferences, occurring on a 5-year cycle, on the dense interstellar medium and related topics. The main results constitute valuable proceedings that offer everyone working in this field an authoritative and comprehensive source of reference.

Interstellar Turbulence

Interstellar Turbulence PDF Author: José Franco
Publisher: Cambridge University Press
ISBN: 9780521651318
Category : Science
Languages : en
Pages : 304

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Book Description
This timely volume presents a series of review articles covering every aspect of interstellar turbulence--from accretion disks, molecular clouds, atomic and ionized media, through to spiral galaxies - based on a major international conference held in Mexico City.With advances in observational techniques and the development of more efficient computer codes and faster computers, research in this area has made spectacular progress in recent years. This book provides a comprehensive overview of the most important developments in observing and modelling turbulent flows in the cosmos. It provides graduate student and researchers with a state-of-the-art summary of observational, theoretical and computational research in interstellar turbulence.

The Labyrinth of Star Formation

The Labyrinth of Star Formation PDF Author: Dimitris Stamatellos
Publisher: Springer Science & Business Media
ISBN: 3319030418
Category : Science
Languages : en
Pages : 490

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Book Description
This volume contains the proceedings from the conference "The Labyrinth of Star Formation" that was held in Crete, Greece, in June 2012, to honour the contributions to the study of star formation made by Professor Anthony Whitworth of Cardiff University. The book covers many aspects of theoretical and observational star formation: low-mass star formation; young circumstellar discs; computational methods; triggered star formation; the stellar initial mass function; high-mass star formation and stellar clusters. Each section starts with a review paper, followed by papers discussing recent theoretical and observational work. This volume summarises our current understanding of star formation and is useful for both graduate students and researchers alike.

The Galaxy Disk in Cosmological Context (IAU S254)

The Galaxy Disk in Cosmological Context (IAU S254) PDF Author: International Astronomical Union. Symposium
Publisher: Cambridge University Press
ISBN: 9780521889858
Category : Science
Languages : en
Pages : 542

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Book Description
The paradigm of a dark energy- and dark matter-dominated Universe, with the hierarchical merger scenario for the formation of galaxies, has scored impressive successes in matching the observed Universe. However, the theory fails to explain the difficulty in generating ordinary disk galaxies such as the Milky Way, suggesting that some important physics must be missing in current models. IAU Symposium 254 was organized to address this question, gathering researchers from an unusually broad range of fields, from cosmology to interstellar matter, and the formation and evolution of stars. High-class reviews, lectures and posters combine to define the frontiers in the field and point the way to new avenues of research. This volume presents a unique set of succinct overviews illuminating the full range of topics in this very active field. It also honors Danish astrophysicist Bengt Strömgren (1908-1987), who laid much of the foundation for this entire field.

The Magellanic System (IAU S256)

The Magellanic System (IAU S256) PDF Author: International Astronomical Union. Symposium
Publisher: Cambridge University Press
ISBN: 9780521889872
Category : Science
Languages : en
Pages : 552

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Book Description
Provides the most complete and up-to-date account of our understanding of the Magellanic Clouds and the astrophysical processes within them.

Astrophysical Hydrodynamics

Astrophysical Hydrodynamics PDF Author: Steven N. Shore
Publisher: John Wiley & Sons
ISBN: 3527619062
Category : Science
Languages : en
Pages : 474

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Book Description
This latest edition of the proven and comprehensive treatment on the topic -- from the bestselling author of "Tapestry of Modern Astrophysics" -- has been updated and revised to reflect the newest research results. Suitable for AS0000 and AS0200 courses, as well as advanced astrophysics and astronomy lectures, this is an indispensable theoretical backup for studies on celestial body formation and astrophysics. Includes exercises with solutions.