Theory of Stellar Atmospheres

Theory of Stellar Atmospheres
Author: Ivan Hubeny
Publisher: Princeton University Press
Total Pages: 945
Release: 2014-10-26
Genre: Science
ISBN: 1400852730

The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses. The book is ideal for astronomers who want to acquire deeper insight into the physical foundations of the theory of stellar atmospheres, or who want to learn about modern computational techniques for treating radiative transfer in non-equilibrium situations. It can also serve as a rigorous yet accessible introduction to the discipline for graduate students. Provides a comprehensive, up-to-date account of the field Covers computational methods as well as the underlying physics Serves as an ideal reference book for researchers and a rigorous yet accessible textbook for graduate students An online illustration package is available to professors at press.princeton.edu

Introduction to Stellar Atmospheres and Interiors

Introduction to Stellar Atmospheres and Interiors
Author: Eva Novotny
Publisher: Oxford University Press, USA
Total Pages: 568
Release: 1973
Genre: Language Arts & Disciplines
ISBN:

Part One of this four-part book reviews the observational data with which the theoretical results must be compared. Parts Two and Three develop the basic theoretical concepts pertinent to stellar atmospheres and interiors. Part Four provides detailed calculations of a model atmosphere and a number of model interiors.

Stellar Atmospheres

Stellar Atmospheres
Author: Cecilia Helena Payne Gaposchkin
Publisher:
Total Pages: 238
Release: 1925
Genre: Astrophysics
ISBN:

Original thesis submitted to Radcliffe College. The typescript is a summary of the thesis with handwritten ink insertions. The galley proof contains the full text and bears blue and graphite pencil markings. A library thesis use form is affixed to the bottom of the first page of the galley.

Selected Papers, Volume 1

Selected Papers, Volume 1
Author: Subrahmanyan Chandrasekhar
Publisher: University of Chicago Press
Total Pages: 540
Release: 1989-04-26
Genre: Science
ISBN: 9780226100906

This is the first of six volumes collecting significant papers of the distinguished astrophysicist and Nobel laureate S. Chandrasekhar. His work is notable for its breadth as well as for its brilliance; his practice has been to change his focus from time to time to pursue new areas of research. The result has been a prolific career full of discoveries and insights, some of which are only now being fully appreciated. Chandrasekhar has selected papers that trace the development of his ideas and that present aspects of his work not fully covered in the books he has periodically published to summarize his research in each area. Volume 1, Stellar Structure and Stellar Atmospheres, covers primarily the period 1930-40 and includes early papers on the theory of white dwarfs. In the Preface, Chandrasekhar explains the criteria for selection and provides historical background. Each subsequent volume will include a foreword by an authority on the topics covered.

Radiative Transfer

Radiative Transfer
Author: Subrahmanyan Chandrasekhar
Publisher: Courier Corporation
Total Pages: 418
Release: 2013-04-15
Genre: Science
ISBN: 0486318451

This book by a Nobel Laureate provides the foundation for analysis of stellar atmospheres, planetary illumination, and sky radiation. Suitable for students and professionals in physics, nuclear physics, astrophysics, and atmospheric studies. 1950 edition.

Theory of Stellar Atmospheres (ARC)

Theory of Stellar Atmospheres (ARC)
Author: Ivan Hubeny
Publisher:
Total Pages: 944
Release:
Genre:
ISBN: 9781400898794

This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses. The book is ideal for astronomers who want to acquire deeper insight into the physical foundations of the theory of stellar atmospheres, or who want to learn about modern computational techniques for treating radiative transfer in non-equilibrium sit.

Exoplanet Atmospheres

Exoplanet Atmospheres
Author: Sara Seager
Publisher: Princeton University Press
Total Pages: 258
Release: 2010-08-02
Genre: Science
ISBN: 1400835305

Over the past twenty years, astronomers have identified hundreds of extrasolar planets--planets orbiting stars other than the sun. Recent research in this burgeoning field has made it possible to observe and measure the atmospheres of these exoplanets. This is the first textbook to describe the basic physical processes--including radiative transfer, molecular absorption, and chemical processes--common to all planetary atmospheres, as well as the transit, eclipse, and thermal phase variation observations that are unique to exoplanets. In each chapter, Sara Seager offers a conceptual introduction, examples that combine the relevant physics equations with real data, and exercises. Topics range from foundational knowledge, such as the origin of atmospheric composition and planetary spectra, to more advanced concepts, such as solutions to the radiative transfer equation, polarization, and molecular and condensate opacities. Since planets vary widely in their atmospheric properties, Seager emphasizes the major physical processes that govern all planetary atmospheres. Moving from first principles to cutting-edge research, Exoplanet Atmospheres is an ideal resource for students and researchers in astronomy and earth sciences, one that will help prepare them for the next generation of planetary science. The first textbook to describe exoplanet atmospheres Illustrates concepts using examples grounded in real data Provides a step-by-step guide to understanding the structure and emergent spectrum of a planetary atmosphere Includes exercises for students

An Introduction to Stellar Astrophysics

An Introduction to Stellar Astrophysics
Author: Francis LeBlanc
Publisher: John Wiley & Sons
Total Pages: 358
Release: 2011-08-24
Genre: Science
ISBN: 1119964970

An Introduction to Stellar Astrophysics aspires to provide the reader with an intermediate knowledge on stars whilst focusing mostly on the explanation of the functioning of stars by using basic physical concepts and observational results. The book is divided into seven chapters, featuring both core and optional content: Basic concepts Stellar Formation Radiative Transfer in Stars Stellar Atmospheres Stellar Interiors Nucleosynthesis and Stellar Evolution and Chemically Peculiar Stars and Diffusion. Student-friendly features include: Detailed examples to help the reader better grasp the most important concepts A list of exercises is given at the end of each chapter and answers to a selection of these are presented. Brief recalls of the most important physical concepts needed to properly understand stars. A summary for each chapter Optional and advanced sections are included which may be skipped without interfering with the flow of the core content. This book is designed to cover the most important aspects of stellar astrophysics inside a one semester (or half-year) course and as such is relevant for advanced undergraduate students following a first course on stellar astrophysics, in physics or astronomy programs. It will also serve as a basic reference for a full-year course as well as for researchers working in related fields.

Stellar Structure and Evolution

Stellar Structure and Evolution
Author: Rudolf Kippenhahn
Publisher: Springer Science & Business Media
Total Pages: 480
Release: 2012-12-06
Genre: Science
ISBN: 3642615236

A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The text presents an overview of the models developed to explain the stability, dynamics and evolution of the stars, and great care is taken to detail the various stages in a star's life. The authors have succeeded in producing a unique text based on their own pioneering work in stellar modeling. Since its publication, this textbook has come to be considered a classic by both readers and teachers in astrophysics. This study edition is intended for students in astronomy and physics alike.