9780750312912 - interstellar flow and star formation (aas-iop astronomy) de vazquez-semadeni, enrique (16 resultados)
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Librería: GreatBookPrices, Columbia, MD, Estados Unidos de AmericaGreatBookPrices
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Librería: GreatBookPricesUK, Woodford Green, Reino UnidoGreatBookPricesUK
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Librería: PBShop.store UK, Fairford, GLOS, Reino UnidoPBShop.store UK
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EUR 126,56
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HRD. Condición: New. New Book. Shipped from UK. Established seller since 2000.
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Librería: GreatBookPrices, Columbia, MD, Estados Unidos de AmericaGreatBookPrices
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EUR 131,37
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Librería: PBShop.store US, Wood Dale, IL, Estados Unidos de AmericaPBShop.store US
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Librería: Grand Eagle Retail, Bensenville, IL, Estados Unidos de AmericaGrand Eagle Retail
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EUR 163,55
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Hardcover. Condición: new. Hardcover. The first part of this book reviews the basic theoretical knowledge necessary to understand the flow of interstellar gas that leads to the formation of stars, including ample discussion of the physical implications, the limitations of standard assumptions, and the necessary extensions for mo…re realistic descriptions. The second part presents a self-consistent view of the process of cloud formation and evolution that leads to the formation of stars, starting from the mechanisms responsible for the formation of clouds in the diffuse interstellar medium, passing through their growth, the onset of gravitational contraction, the onset of star formation, and culminating on the dispersal of the star-forming regions and the properties of the star clusters formed by this process. Throughout the book, special emphasis is made on the fluid nature of the interstellar medium.Key features:Provides comprehensive description of the physics (compressible and incompressible turbulence, thermodynamics, self-gravity, and some aspects of magnetic fields) needed to describe the flow of interstellar gas and the resulting star formation process from a collective (i.e., not individual) point of view.Addresses nonlinear processes (turbulence, cooling) and the interplay between them and self-gravity, towards star formation.Includes extensive qualitative and interpretative discussion of the theory, directed to graduate students and professional astronomers not familiar with the details and implications.Discussion of frequent misconceptions and misinterpretations of the theory, and the importance of the continuum nature of the interstellar medium.Discussion of relevant results from early times that are often overlooked in current literature. An insightful discussion of the basic physics underlying interstellar cloud formation and evolution, going beyond traditional but incomplete or unrealistic applications and emphasizing the continuum nature of the interstellar medium, followed by a unified account of the life cycle of interstellar clouds and their star-forming activity. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.
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Librería: Rarewaves.com USA, London, LONDO, Reino UnidoRarewaves.com USA
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EUR 163,76
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Hardback. Condición: New.
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Librería: Ria Christie Collections, Uxbridge, Reino UnidoRia Christie Collections
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EUR 151,99
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Librería: THE SAINT BOOKSTORE, Southport, , Reino UnidoTHE SAINT BOOKSTORE
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EUR 163,87
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Hardback. Condición: New. New copy - Usually dispatched within 4 working days.
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Librería: moluna, Greven, , Alemaniamoluna
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EUR 137,38
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Gebunden. Condición: New.
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Librería: CitiRetail, Stevenage, Reino UnidoCitiRetail
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EUR 153,63
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Hardcover. Condición: new. Hardcover. The first part of this book reviews the basic theoretical knowledge necessary to understand the flow of interstellar gas that leads to the formation of stars, including ample discussion of the physical implications, the limitations of standard assumptions, and the necessary extensions for mo…re realistic descriptions. The second part presents a self-consistent view of the process of cloud formation and evolution that leads to the formation of stars, starting from the mechanisms responsible for the formation of clouds in the diffuse interstellar medium, passing through their growth, the onset of gravitational contraction, the onset of star formation, and culminating on the dispersal of the star-forming regions and the properties of the star clusters formed by this process. Throughout the book, special emphasis is made on the fluid nature of the interstellar medium.Key features:Provides comprehensive description of the physics (compressible and incompressible turbulence, thermodynamics, self-gravity, and some aspects of magnetic fields) needed to describe the flow of interstellar gas and the resulting star formation process from a collective (i.e., not individual) point of view.Addresses nonlinear processes (turbulence, cooling) and the interplay between them and self-gravity, towards star formation.Includes extensive qualitative and interpretative discussion of the theory, directed to graduate students and professional astronomers not familiar with the details and implications.Discussion of frequent misconceptions and misinterpretations of the theory, and the importance of the continuum nature of the interstellar medium.Discussion of relevant results from early times that are often overlooked in current literature. An insightful discussion of the basic physics underlying interstellar cloud formation and evolution, going beyond traditional but incomplete or unrealistic applications and emphasizing the continuum nature of the interstellar medium, followed by a unified account of the life cycle of interstellar clouds and their star-forming activity. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.
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Librería: California Books, Miami, FL, Estados Unidos de AmericaCalifornia Books
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EUR 199,61
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Condición: New.
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Librería: Rarewaves.com UK, London, Reino UnidoRarewaves.com UK
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EUR 154,92
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Hardback. Condición: New.
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Librería: AHA-BUCH GmbH, Einbeck, AlemaniaAHA-BUCH GmbH
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EUR 171,52
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Buch. Condición: Neu. Neuware - The first part of this book reviews the basic theoretical knowledge necessary to understand the flow of interstellar gas that leads to the formation of stars, including ample discussion of the physical implications, the limitations of standard assumptions, and the necessary extensions for more rea…listic descriptions. The second part presents a self-consistent view of the process of cloud formation and evolution that leads to the formation of stars, starting from the mechanisms responsible for the formation of clouds in the diffuse interstellar medium, passing through their growth, the onset of gravitational contraction, the onset of star formation, and culminating on the dispersal of the star-forming regions and the properties of the star clusters formed by this process. Throughout the book, special emphasis is made on the fluid nature of the interstellar medium.
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Librería: AussieBookSeller, Truganina, VIC, AustraliaAussieBookSeller
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EUR 243,00
Envío por EUR 31,87Se envía de Australia a Estados Unidos de AmericaCantidad disponible: 1 disponibles
Hardcover. Condición: new. Hardcover. The first part of this book reviews the basic theoretical knowledge necessary to understand the flow of interstellar gas that leads to the formation of stars, including ample discussion of the physical implications, the limitations of standard assumptions, and the necessary extensions for mo…re realistic descriptions. The second part presents a self-consistent view of the process of cloud formation and evolution that leads to the formation of stars, starting from the mechanisms responsible for the formation of clouds in the diffuse interstellar medium, passing through their growth, the onset of gravitational contraction, the onset of star formation, and culminating on the dispersal of the star-forming regions and the properties of the star clusters formed by this process. Throughout the book, special emphasis is made on the fluid nature of the interstellar medium.Key features:Provides comprehensive description of the physics (compressible and incompressible turbulence, thermodynamics, self-gravity, and some aspects of magnetic fields) needed to describe the flow of interstellar gas and the resulting star formation process from a collective (i.e., not individual) point of view.Addresses nonlinear processes (turbulence, cooling) and the interplay between them and self-gravity, towards star formation.Includes extensive qualitative and interpretative discussion of the theory, directed to graduate students and professional astronomers not familiar with the details and implications.Discussion of frequent misconceptions and misinterpretations of the theory, and the importance of the continuum nature of the interstellar medium.Discussion of relevant results from early times that are often overlooked in current literature. An insightful discussion of the basic physics underlying interstellar cloud formation and evolution, going beyond traditional but incomplete or unrealistic applications and emphasizing the continuum nature of the interstellar medium, followed by a unified account of the life cycle of interstellar clouds and their star-forming activity. Shipping may be from our Sydney, NSW warehouse or from our UK or US warehouse, depending on stock availability.
