hardcover. Condizione: Good.
Da: GreatBookPrices, Columbia, MD, U.S.A.
EUR 114,93
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Aggiungi al carrelloCondizione: New.
Da: California Books, Miami, FL, U.S.A.
EUR 117,29
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Aggiungi al carrelloCondizione: New.
Condizione: As New. Unread book in perfect condition.
Da: Ria Christie Collections, Uxbridge, Regno Unito
EUR 115,49
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Aggiungi al carrelloCondizione: New. In.
Da: GreatBookPricesUK, Woodford Green, Regno Unito
EUR 115,48
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Aggiungi al carrelloCondizione: New.
Da: GreatBookPrices, Columbia, MD, U.S.A.
Condizione: New.
Condizione: New.
Da: Ria Christie Collections, Uxbridge, Regno Unito
EUR 127,69
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Aggiungi al carrelloCondizione: New. In.
Condizione: New. pp. 376 Softcover reprint of the original 1st ed. 2015 edition NO-PA16APR2015-KAP.
Condizione: New. pp. 322.
Condizione: New. pp. 322.
Lingua: Inglese
Editore: Springer Berlin Heidelberg, 2003
ISBN 10: 354040838X ISBN 13: 9783540408383
Da: moluna, Greven, Germania
EUR 115,61
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Aggiungi al carrelloCondizione: New. This book contains the expanded lecture notes of the 32nd Saas-Fee Advanced Course. The three contributions present the central themes in modern research on the cold universe, ranging from cold objects at large distances to the physics of dust in cold cl.
Da: preigu, Osnabrück, Germania
EUR 95,15
Quantità: 5 disponibili
Aggiungi al carrelloTaschenbuch. Condizione: Neu. The Cold Universe | Saas-Fee Advanced Course 32, 2002. Swiss Society for Astrophysics and Astronomy | Andrew W. Blain (u. a.) | Taschenbuch | xiv | Englisch | 2010 | Springer | EAN 9783642074073 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Da: Ria Christie Collections, Uxbridge, Regno Unito
EUR 159,44
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Aggiungi al carrelloCondizione: New. In.
Lingua: Inglese
Editore: Springer, Springer Berlin Heidelberg, 2010
ISBN 10: 3642074073 ISBN 13: 9783642074073
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 106,99
Quantità: 1 disponibili
Aggiungi al carrelloTaschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - Modern astronomy has stretched its domains of exploration tremendously. Not only objects at very large distances and very old states of the Universe can be examined, but also all kinds of radiations and phenomena are now accessible. Astronomers constantly move from considerations about very - luted to very dense systems. Hot and energetic systems, being the easiest to observe, have attracted a lot of attention. However the cold and low energetic states have been so- what neglected, either because being harder to observe they appear unexc- ing, or because being less well known they tend to be ignored. However the Universe background radiation has now been determined as the most perfect known case of a black-body spectrum, a substantial fraction of matter spends some time close to the temperature of this universal thermal bath, before - ingtransformedintostarsorplanets. Someobjects,suchasrapidlyexpanding gas shells in planetary nebulae, may even succeed in reaching a temperature well below the background radiation temperature through the mere action of adiabatic expansion. In view of the highly dynamical and turbulent state of the interstellar medium, hot and cold temperature uctuations must be expected, while the clear observational bias is to observe the hot rather than the cold uctuations. Fortunately with the accessibility of far-infrared and sub-millimetric instruments such as SCUBA, WMAP, Planck or ALMA, we can expect in the coming years continuous advances in our understanding of these harder to observe cold stages of matter.
Da: Ria Christie Collections, Uxbridge, Regno Unito
EUR 164,32
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Aggiungi al carrelloCondizione: New. In.
Da: preigu, Osnabrück, Germania
EUR 104,15
Quantità: 5 disponibili
Aggiungi al carrelloTaschenbuch. Condizione: Neu. Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality | Saas-Fee Advanced Course 43. Swiss Society for Astrophysics and Astronomy | Nickolay Y. Gnedin (u. a.) | Taschenbuch | Saas-Fee Advanced Course | xi | Englisch | 2016 | Springer | EAN 9783662516768 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Condizione: New.
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 122,12
Quantità: 1 disponibili
Aggiungi al carrelloTaschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book contains the elaborated and updated versions of the 24 lectures given at the 43rd Saas-Fee Advanced Course. Written by four eminent scientists in the field, the book reviews the physical processes related to star formation, starting from cosmologicaldown to galactic scales. It presents a detailed description of the interstellar medium and its link with the star formation. And it describes the main numerical computational techniques designed to solve the equations governing self-gravitating fluids used for modelling of galactic and extra-galactic systems. This book provides a unique framework which is needed to develop and improve the simulation techniques designed for understanding the formation and evolution of galaxies. Presented in an accessible manner it contains the present day state of knowledge of the field. It serves as an entry point and key reference to students and researchers in astronomy, cosmology, and physics.
Da: GreatBookPricesUK, Woodford Green, Regno Unito
EUR 174,03
Quantità: Più di 20 disponibili
Aggiungi al carrelloCondizione: As New. Unread book in perfect condition.
Da: Mispah books, Redhill, SURRE, Regno Unito
EUR 164,50
Quantità: 1 disponibili
Aggiungi al carrelloHardcover. Condizione: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.
Da: GreatBookPrices, Columbia, MD, U.S.A.
EUR 197,39
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Aggiungi al carrelloCondizione: As New. Unread book in perfect condition.
Lingua: Inglese
Editore: Springer, Berlin, Springer, 2003
ISBN 10: 354040838X ISBN 13: 9783540408383
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 142,80
Quantità: 2 disponibili
Aggiungi al carrelloBuch. Condizione: Neu. Neuware - Modern astronomy has stretched its domains of exploration tremendously. Not only objects at very large distances and very old states of the Universe can be examined, but also all kinds of radiations and phenomena are now accessible. Astronomers constantly move from considerations about very - luted to very dense systems. Hot and energetic systems, being the easiest to observe, have attracted a lot of attention. However the cold and low energetic states have been so- what neglected, either because being harder to observe they appear unexc- ing, or because being less well known they tend to be ignored. However the Universe background radiation has now been determined as the most perfect known case of a black-body spectrum, a substantial fraction of matter spends some time close to the temperature of this universal thermal bath, before - ingtransformedintostarsorplanets. Someobjects,suchasrapidlyexpanding gas shells in planetary nebulae, may even succeed in reaching a temperature well below the background radiation temperature through the mere action of adiabatic expansion. In view of the highly dynamical and turbulent state of the interstellar medium, hot and cold temperature uctuations must be expected, while the clear observational bias is to observe the hot rather than the cold uctuations. Fortunately with the accessibility of far-infrared and sub-millimetric instruments such as SCUBA, WMAP, Planck or ALMA, we can expect in the coming years continuous advances in our understanding of these harder to observe cold stages of matter.
Condizione: New. pp. 377.
Da: AHA-BUCH GmbH, Einbeck, Germania
EUR 160,49
Quantità: 1 disponibili
Aggiungi al carrelloBuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book contains the elaborated and updated versions of the 24 lectures given at the 43rd Saas-Fee Advanced Course. Written by four eminent scientists in the field, the book reviews the physical processes related to star formation, starting from cosmologicaldown to galactic scales. It presents a detailed description of the interstellar medium and its link with the star formation. And it describes the main numerical computational techniques designed to solve the equations governing self-gravitating fluids used for modelling of galactic and extra-galactic systems. This book provides a unique framework which is needed to develop and improve the simulation techniques designed for understanding the formation and evolution of galaxies. Presented in an accessible manner it contains the present day state of knowledge of the field. It serves as an entry point and key reference to students and researchers in astronomy, cosmology, and physics.
Da: Mispah books, Redhill, SURRE, Regno Unito
EUR 206,23
Quantità: 1 disponibili
Aggiungi al carrelloPaperback. Condizione: Like New. Like New. book.
Da: GreatBookPrices, Columbia, MD, U.S.A.
Condizione: As New. Unread book in perfect condition.
Da: Revaluation Books, Exeter, Regno Unito
EUR 236,68
Quantità: 2 disponibili
Aggiungi al carrelloHardcover. Condizione: Brand New. 380 pages. 9.50x6.50x1.25 inches. In Stock.
Da: Mispah books, Redhill, SURRE, Regno Unito
EUR 228,88
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Aggiungi al carrelloHardcover. Condizione: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.