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Book Theory of Stellar Atmospheres

Download or read book Theory of Stellar Atmospheres written by Ivan Hubeny and published by Princeton University Press. This book was released on 2014-10-26 with total page 944 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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

Book Theory of Stellar Atmospheres  ARC

Download or read book Theory of Stellar Atmospheres ARC written by Ivan Hubeny and published by . This book was released on with total page 944 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Book Stellar Atmospheres  Theory and Observations

Download or read book Stellar Atmospheres Theory and Observations written by Jean P.de Greve and published by Springer. This book was released on 1997-10-15 with total page 376 pages. Available in PDF, EPUB and Kindle. Book excerpt: The 1996 Summer School of the European Astrophysical Doctoral Network dealt with the atmospheres of stars, the various theories that describe their structure and the interactions with the interior of the stars as well as with the interstellar environment, and the observations that support, modify and sometimes contradict these theories. This volume aims to provide the reader with an insight into problems related to stellar atmospheres both for cool and for hot stars. Furthermore it offers opportunities to deal with modern technologies in analysing observational data versus theoretical modelling.

Book The Theory of Stellar Spectra

Download or read book The Theory of Stellar Spectra written by Charles R. Cowley and published by Routledge. This book was released on 1970 with total page 284 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Theory of the Stellar Atmospheres

Download or read book Theory of the Stellar Atmospheres written by Dimitri Mihalas and published by . This book was released on 1971 with total page 312 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Stellar Atmospheres

Download or read book Stellar Atmospheres written by Cecilia Helena Payne Gaposchkin and published by . This book was released on 1925 with total page 238 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Book Determination of Atmospheric Parameters of B   A   F  and G Type Stars

Download or read book Determination of Atmospheric Parameters of B A F and G Type Stars written by Ewa Niemczura and published by Springer. This book was released on 2014-07-10 with total page 312 pages. Available in PDF, EPUB and Kindle. Book excerpt: This book introduces the theory of stellar atmospheres. Almost everything we know about stars is by analysis of the radiation coming from their atmospheres. Several aspects of astrophysics require accurate atmospheric parameters and abundances. Spectroscopy is one of the most powerful tools at an astronomer’s disposal, allowing the determination of the fundamental parameters of stars: surface temperature, gravity, chemical composition, magnetic field, rotation and turbulence. These can be supplemented by distance measurements or pulsation parameters providing information about stellar interior and stellar evolution, otherwise unavailable. The volume is based on lectures presented at the Wrocław's Spectroscopic School aimed at training young researchers in performing quantitative spectral analysis of low-, mid-, and high-resolution spectra of B, A, and F-type stars.

Book Stellar Atmospheres  Beyond Classical Models

Download or read book Stellar Atmospheres Beyond Classical Models written by L. Crivellari and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 459 pages. Available in PDF, EPUB and Kindle. Book excerpt: The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provided a vital stimulus in the early stages of quantum theory and atomic physics; even today topics such as low-temperature dielectronic recombination develop hand in hand with the interpretation of stellar and nebular spectra. Early work on MHD was similiarly motivated. Many such connections remain to be explored.

Book Problems of Radiative Transfer in the Theory of Stellar Atmospheres

Download or read book Problems of Radiative Transfer in the Theory of Stellar Atmospheres written by Guido Münch and published by . This book was released on 1945 with total page 34 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book Radiative Transfer in Stellar and Planetary Atmospheres

Download or read book Radiative Transfer in Stellar and Planetary Atmospheres written by Lucio Crivellari and published by Cambridge University Press. This book was released on 2020-01-09 with total page 251 pages. Available in PDF, EPUB and Kindle. Book excerpt: Radiative transfer is essential for obtaining information from the spectra of astrophysical objects. This volume provides an overview of the physical and mathematical background of radiative transfer, and its applications to stellar and planetary atmospheres. It covers the phenomenology and physics of early-type and late-type stars, as well as ultra-cool dwarf stars and extrasolar planets. Importantly, it provides a bridge between classical radiative transfer and stellar atmosphere modelling and novel approaches, from both theoretical and computational standpoints. With new fields of application and a dramatic improvement in both observational and computational facilities, it also discusses the future outlook for the field. Chapters are written by eminent researchers from across the astronomical disciplines where radiative transfer is employed. Using the most recent observations, this is a go-to resource for graduate students and researchers in astrophysics.

Book Introduction to Stellar Atmospheres and Interiors

Download or read book Introduction to Stellar Atmospheres and Interiors written by Eva Novotny and published by Oxford University Press, USA. This book was released on 1973 with total page 568 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Book Selected Papers  Volume 1

    Book Details:
  • Author : Subrahmanyan Chandrasekhar
  • Publisher : University of Chicago Press
  • Release : 1989-04-26
  • ISBN : 9780226100906
  • Pages : 540 pages

Download or read book Selected Papers Volume 1 written by Subrahmanyan Chandrasekhar and published by University of Chicago Press. This book was released on 1989-04-26 with total page 540 pages. Available in PDF, EPUB and Kindle. Book excerpt: 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.

Book Theory of the Stellar Atmospheres

Download or read book Theory of the Stellar Atmospheres written by Dimitri Mihalas and published by . This book was released on 1971 with total page 312 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book The Theory of Stellar Atmospheres

Download or read book The Theory of Stellar Atmospheres written by Charles A. Whitney and published by . This book was released on with total page 285 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Book The Observation and Analysis of Stellar Photospheres

Download or read book The Observation and Analysis of Stellar Photospheres written by David F. Gray and published by Cambridge University Press. This book was released on 2005-11-17 with total page 560 pages. Available in PDF, EPUB and Kindle. Book excerpt: Third edition textbook for use on advanced courses on stellar physics.

Book Theoretical Research on Stellar Atmospheres

Download or read book Theoretical Research on Stellar Atmospheres written by Charles Allen Whitney and published by . This book was released on 1967 with total page 88 pages. Available in PDF, EPUB and Kindle. Book excerpt: A brief sketch of the development of the theory of stellar atmospheres since 1920 is followed by a discussion of problems that may be central to this theory during the next 5 years. The second section provides an annotated bibliography of theoretical work performed at Harvard College Observatory and Smithsonian Astrophysical Observatory during the decade 1957-1967.