Author: Charles R. Cowley
Publisher: Routledge
ISBN:
Category : Science
Languages : en
Pages : 284
Book Description
The Theory of Stellar Spectra
Author: Charles R. Cowley
Publisher: Routledge
ISBN:
Category : Science
Languages : en
Pages : 284
Book Description
Publisher: Routledge
ISBN:
Category : Science
Languages : en
Pages : 284
Book Description
Theory of Stellar Atmospheres
Author: Ivan Hubeny
Publisher: Princeton University Press
ISBN: 0691163294
Category : Science
Languages : en
Pages : 944
Book Description
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
Publisher: Princeton University Press
ISBN: 0691163294
Category : Science
Languages : en
Pages : 944
Book Description
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
Theory of Stellar Spectra
Author: Viktor Viktorovich Sobolev
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 292
Book Description
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 292
Book Description
On a Physical Theory of Stellar Spectra
Author: M. N.. Saha
Publisher:
ISBN:
Category :
Languages : en
Pages : 19
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 19
Book Description
Theory of Stellar Spectra [with Lists of References]
Author:
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 279
Book Description
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 279
Book Description
Theory of Stellar Spectra
Author: Viktor Viktorovič Sobolev
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 279
Book Description
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 279
Book Description
Spectroscopy: The Key to the Stars
Author: Keith Robinson
Publisher: Springer Science & Business Media
ISBN: 0387682880
Category : Science
Languages : en
Pages : 165
Book Description
This is the first non-technical book on spectroscopy written specifically for practical amateur astronomers. It includes all the science necessary for a qualitative understanding of stellar spectra, but avoids a mathematical treatment which would alienate many of its intended readers. Any amateur astronomer who carries out observational spectroscopy and who wants a non-technical account of the physical processes which determine the intensity and profile morphology of lines in stellar spectra will find this is the only book written specially for them. It is an ideal companion to existing books on observational amateur astronomical spectroscopy.
Publisher: Springer Science & Business Media
ISBN: 0387682880
Category : Science
Languages : en
Pages : 165
Book Description
This is the first non-technical book on spectroscopy written specifically for practical amateur astronomers. It includes all the science necessary for a qualitative understanding of stellar spectra, but avoids a mathematical treatment which would alienate many of its intended readers. Any amateur astronomer who carries out observational spectroscopy and who wants a non-technical account of the physical processes which determine the intensity and profile morphology of lines in stellar spectra will find this is the only book written specially for them. It is an ideal companion to existing books on observational amateur astronomical spectroscopy.
Contribution to Spectral Type Theory
Author:
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 54
Book Description
Publisher:
ISBN:
Category : Stars
Languages : en
Pages : 54
Book Description
Stellar Atmospheres
Author: Cecilia Helena Payne Gaposchkin
Publisher:
ISBN:
Category : Astrophysics
Languages : en
Pages : 238
Book Description
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.
Publisher:
ISBN:
Category : Astrophysics
Languages : en
Pages : 238
Book Description
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.
Theory of Stellar Atmospheres
Author: Ivan Hubeny
Publisher: Princeton University Press
ISBN: 1400852730
Category : Science
Languages : en
Pages : 944
Book Description
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
Publisher: Princeton University Press
ISBN: 1400852730
Category : Science
Languages : en
Pages : 944
Book Description
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