mathias scholz (89 risultati)

Condizione: very good. Gut/Very good: Buch bzw. Schutzumschlag mit wenigen Gebrauchsspuren an Einband, Schutzumschlag oder Seiten. / Describes a book or dust jacket that does show some signs of wear on either the binding, dust jacket or pages.

Hardcover. Condizione: Très bon. Ancien livre de bibliothèque avec équipements. Edition 2011. Ammareal reverse jusqu'à 15% du prix net de cet article à des organisations caritatives. ENGLISH DESCRIPTION Book Condition: Used, Very good. Former library book. Edition 2011. Ammareal gives back up to 15% of this item's net price to charity organizations.

Condizione: New. In.

482 S. : graph. Darst. ; 24 cm + 1 CD-ROM ISBN 9783800144273 Der Versand erfolgt innerhalb von 2 Werktagen. Bei Gewicht - wird bei Buchtitel angezeigt - ab 1000 Gramm = 7 Euro Portoanteil in D., EU = 20 Euro, WE LT B I T T E V O R BESTELLUNG ERFRAGEN! Über 2000 Titel wurden wegen Lagerauflösung reduziert - erkennbar meist an der Preisendziffer "9". NO DELIVERY TO THE UNITED STATES FOR US POSSIBLE!! Sprache: Deutsch Gewicht in Gramm: 1400 Gebundener Originalpappband.Wohl ungelesenes Exemplar.

Paperback. Condizione: Brand New. 156 pages. German language. 9.00x6.00x0.39 inches. In Stock.

Paperback. Condizione: Brand New. 325 pages. German language. 9.00x6.00x0.82 inches. In Stock.

Softcover/Paperback. 482 Seiten mit 174 Abbildungen und 56 Tabellen und einer CD-ROM Unterer Buchschnitt mit leichtem Berieb und ein wenig an dieser Stelle angeschmutzt. Ansonsten in einem guten Zustand. A3/104 Sprache: Deutsch Gewicht in Gramm: 1270.

Paperback. Condizione: Brand New. 184 pages. German language. 8.27x5.83x0.42 inches. In Stock.

Paperback. Condizione: Brand New. 174 pages. German language. 8.27x5.83x0.40 inches. In Stock.

Paperback. Condizione: Brand New. 96 pages. German language. 9.00x6.00x0.24 inches. In Stock.

Condizione: Wie neu. 4. 174 S. Alle Bücher & Medienartikel von Book Broker sind stets in gutem & sehr gutem gebrauchsfähigen Zustand. Unser Produktfoto entspricht dem hier angebotenen Artikel, dieser weist folgende Merkmale auf: Helle/saubere Seiten in fester Bindung. 1. Auflage 2014 Sprache: Deutsch Gewicht in Gramm: 290 Taschenbuch, Maße: 14.81 cm x 1.02 cm x 21.01 cm.

paperback. Condizione: Very Good.

Condizione: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide.

Condizione: New. 2024th edition NO-PA16APR2015-KAP.

Condizione: New. Brand New Original US Edition. Customer service! Satisfaction Guaranteed.

Condizione: New. Brand New Original US Edition. Customer service! Satisfaction Guaranteed.

Condizione: New.

paperback. Condizione: Very Good.

Condizione: New.

Paperback. Condizione: Brand New. 165 pages. German language. 8.00x5.25x0.39 inches. In Stock.

Taschenbuch. Condizione: Neu. Neuware - Panopticon - A Journey of Discovery through the Universe of Knowledge.

Paperback. Condizione: new. Paperback. Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He studied physics at the University of Rostock from 1981 to 1986.Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future. Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. Shipping may be from multiple locations in the US or from the UK, depending on stock availability.

EA. sehr guter Zustand, 380 S., Grossformat, Pappband, geb. Erstausgabe. Weitere HerausgeberInnen: Sabine Stab, Frank Dziock, Klaus Henle. Mit 96 Abbildungen und 31 Tabellen. Massgebliche Untersuchung zum Thema. Konzepte für die nachhaltige Entwicklung einer Flusslandschaft Band 4 Gramm 600.

Hardcover. Condizione: New.

Condizione: Very Good.

Condizione: New. In.

Paperback. Condizione: New.

Paperback. Condizione: new. Paperback. Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholz is hobby astronomer. He studied physics at the University of Rostock from 1981 to 1986.Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future. Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. Shipping may be from our UK warehouse or from our Australian or US warehouses, depending on stock availability.

Taschenbuch. Condizione: Neu. The Physics of Stars | Structure, Evolution and Properties | Mathias Scholz | Taschenbuch | x | Englisch | 2025 | Springer | EAN 9783662700150 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.

Taschenbuch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.Mathias Scholzis hobby astronomer. Hestudied physics at the University of Rostock from 1981 to 1986.Interested students in the natural and engineering sciences, as well as high school graduates, instructors, teachers, and amateur astronomers, will find a valuable overview of the physics of stars in this book. The only prerequisite is a basic mathematical and physical background, which does not go beyond the knowledge of integral and differential calculus. In this regard, this book aims to bridge the gap with the specialized literature available on the internet, allowing readers to benefit from it.The first part traces the historical development that led to a detailed understanding of the nature of stars and their life cycles. The goal of the following chapters is to provide a pragmatic introduction to the physical processes that determine the structure and evolution of stars based on their fundamental parameters such as mass and chemical composition. It will show what can be learned from the analysis of starlight about stellar atmospheres, the fundamental role of the virial theorem in the lives of stars, and the nuclear processes deep inside stars that provide the energy that makes them shine. Finally, there will be an in-depth phenomenological look at the final stages of stellar evolution. This section will discuss states of matter that are far from experimental realization but whose properties can be, at least in principle, inferred from the observation of concrete objects such as white dwarfs or neutron stars. Exciting developments are still expected in this area in the future.