Beckman j e crivellari l (15 résultats)

Hardcover. Etat : Very Good. Exlibrary with usual markings, stickers, & stamps. Cover soiled. All pages clean. Edge soiled. Progress in Stellar Spectral Line Formation Theory (NATO Advanced Study Institute Series) brings together leading astrophysicists to examine the state of the art in modeling how spectral lines form in stellar atmospheres. The volume covers radiative transfer, non‑LTE effects, line broadening mechanisms, convection and turbulence, opacity sources, and the computational methods used to interpret stellar spectra. It captures a moment when stellar‑atmosphere theory was rapidly advancing, integrating improved physics with emerging numerical techniques to refine our understanding of stellar structure, composition, and evolution. 🎯 Ideal For Researchers in astrophysics, stellar atmospheres, radiative transfer, and spectroscopy Graduate students working on line‑formation modeling, stellar diagnostics, or non‑LTE theory Observatories and institutional libraries building collections in stellar physics and spectral analysis Collectors of NATO ASI volumes, especially those in astrophysics and space science Anyone curating a thematic archive on stellar modeling, spectral diagnostics, or computational astrophysics ⭐ Why It Matters Provides primary‑source research from a major international workshop — invaluable for understanding how stellar‑line theory evolved Offers detailed treatments of non‑LTE processes, broadening physics, and radiative‑transfer methods that remain foundational NATO ASI volumes often had limited print runs, making intact copies increasingly desirable Bridges observational astronomy with theoretical modeling, giving researchers a comprehensive view of the field's development Strengthens any curated archive focused on stellar spectroscopy, astrophysical modeling, or the history of stellar‑atmosphere theory.…

Etat : Very Good. 1985th Edition. Former library copy. Pages intact with possible writing/highlighting. Binding strong with minor wear. Dust jackets/supplements may not be included. Includes library markings. Stock photo provided. Product includes identifying sticker. Better World Books: Buy Books. Do Good. …

Etat : As New. Unread book in perfect condition.

Etat : New.

Etat : New. pp. 468 Index.

Paperback. Etat : Brand New. 468 pages. 9.25x6.10x1.06 inches. In Stock.

Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost enti rely from line analysis, as does a major fraction of our ability to model stellar atmospheres. As new facets of the universe become observable so the techniques of high reso lution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars. Fabry-Perot interferometers and their modern deriva tives are bringing new ranges of resolving power to studies of atomic and ionic interstellar lines, and of course radio techniques imply exceedingly high resolution for the cool interstellar medium of molecules and radicals. Telescopes in space are extending the spectral range of these types of observations. Already the Copernicus and IUE high resolution spectrographs have given us a tantalizing glimmer of what it will be like to obtain ultraviolet spectra with resolution and signal to noise ratio approaching those obtainable on the ground. Fairly soon Space Telescope will be producing high resolution spectroscopic data of unparal leled quali ty and distance range. As often happens in astro physics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data.…

Hardcover. Etat : Very Good. No Jacket. Hardcover 1985 edition. Ex-library book with stamps and labels attached. Binding firm. Pages unmarked and clean. Covers and text in very good condition. Series: NATO ASI series. Series C: Mathematical and Physical Sciences ;Vol. 152. [xvi, 448 p. : ill. ; 25 cm].…

Etat : new. Questo è un articolo print on demand.

PF. Etat : New. This item is printed on demand. Brand new book, sourced directly from publisher. Dispatch time is 6-7 days from our warehouse. Book will be sent in robust, secure packaging to ensure it reaches you securely.

Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost enti rely from line analysis, as does a major fraction of our ability to model stellar atmospheres. As new facets of the universe become observable so the techniques of high reso lution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars. Fabry-Perot interferometers and their modern deriva tives are bringing new ranges of resolving power to studies of atomic and ionic interstellar lines, and of course radio techniques imply exceedingly high resolution for the cool interstellar medium of molecules and radicals. Telescopes in space are extending the spectral range of these types of observations. Already the Copernicus and IUE high resolution spectrographs have given us a tantalizing glimmer of what it will be like to obtain ultraviolet spectra with resolution and signal to noise ratio approaching those obtainable on the ground. Fairly soon Space Telescope will be producing high resolution spectroscopic data of unparal leled quali ty and distance range. As often happens in astro physics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data. 468 pp. Englisch.…

Etat : New. Print on Demand pp. 468 Figures, 49:B&W 6.14 x 9.21 in or 234 x 156 mm (Royal 8vo) Perfect Bound on White w/Gloss Lam.

Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advanced Research Workshop, Grignano-Miramare, Trieste, Italy, September 4-7, 1984 Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar con.…

Etat : New. PRINT ON DEMAND pp. 468.

Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost enti rely from line analysis, as does a major fraction of our ability to model stellar atmospheres. As new facets of the universe become observable so the techniques of high reso lution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employ ing detectors of high quantum efficiency, have revolutioned our ability to observe high quality line profiles, although until now this ability has been confined to the brightest stars. Fabry-Perot interferometers and their modern deriva tives are bringing new ranges of resolving power to studies of atomic and ionic interstellar lines, and of course radio techniques imply exceedingly high resolution for the cool interstellar medium of molecules and radicals. Telescopes in space are extending the spectral range of these types of observations. Already the Copernicus and IUE high resolution spectrographs have given us a tantalizing glimmer of what it will be like to obtain ultraviolet spectra with resolution and signal to noise ratio approaching those obtainable on the ground. Fairly soon Space Telescope will be producing high resolution spectroscopic data of unparal leled quali ty and distance range. As often happens in astro physics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 468 pp. Englisch.…