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Progress in Stellar Spectral Line Formation Theory (Paperback, Softcover reprint of the original 1st ed. 1985) Loot Price: R1,454
Discovery Miles 14 540
Progress in Stellar Spectral Line Formation Theory (Paperback, Softcover reprint of the original 1st ed. 1985): J.E. Beckman,...

Progress in Stellar Spectral Line Formation Theory (Paperback, Softcover reprint of the original 1st ed. 1985)

J.E. Beckman, L. Crivellari

Series: NATO Science Series C, 152

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Loot Price R1,454 Discovery Miles 14 540 | Repayment Terms: R136 pm x 12*

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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."

General

Imprint: Springer
Country of origin: Netherlands
Series: NATO Science Series C, 152
Release date: November 2011
First published: 1985
Editors: J.E. Beckman • L. Crivellari
Dimensions: 235 x 155 x 23mm (L x W x T)
Format: Paperback
Pages: 464
Edition: Softcover reprint of the original 1st ed. 1985
ISBN-13: 978-9401088701
Categories: Books > Science & Mathematics > Astronomy, space & time > General
Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
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LSN: 9401088705
Barcode: 9789401088701

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