Progress in Stellar Spectral Line Formation Theory:
Gespeichert in:
| Weitere Verfasser: | , |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1985
|
| Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
152 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost entirely 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 resolution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employing 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 derivatives 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 unparalleled quality and distance range. As often happens in astrophysics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data |
| Beschreibung: | 1 Online-Ressource (464p) |
| ISBN: | 9789400953727 9789401088701 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-009-5372-7 |
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| 245 | 1 | 0 | |a Progress in Stellar Spectral Line Formation Theory |c edited by John E. Beckman, Lucio Crivellari |
| 246 | 1 | 3 | |a Proceedings of the NATO Advanced Research Workshop, Grignano-Miramare, Trieste, Italy, September 4-7, 1984 |
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| 490 | 1 | |a NATO ASI Series, Series C: Mathematical and Physical Sciences |v 152 |x 1389-2185 | |
| 500 | |a Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost entirely 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 resolution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employing 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 derivatives 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 unparalleled quality and distance range. As often happens in astrophysics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data | ||
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Datensatz im Suchindex
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|---|---|
| any_adam_object | |
| author2 | Beckman, John E. Crivellari, Lucio |
| author2_role | edt edt |
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| author_facet | Beckman, John E. Crivellari, Lucio |
| building | Verbundindex |
| bvnumber | BV042415232 |
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| dewey-full | 523.01 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.01 |
| dewey-search | 523.01 |
| dewey-sort | 3523.01 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-5372-7 |
| format | Electronic eBook |
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| spelling | Beckman, John E. edt Progress in Stellar Spectral Line Formation Theory edited by John E. Beckman, Lucio Crivellari Proceedings of the NATO Advanced Research Workshop, Grignano-Miramare, Trieste, Italy, September 4-7, 1984 Dordrecht Springer Netherlands 1985 1 Online-Ressource (464p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 152 1389-2185 Spectral line formation theory is at the heart of astrophysical diagnostic. Our knowledge of abundances, in both stellar and interstellar contexts, comes almost entirely 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 resolution spectroscopy are brought to bear, with great reward. Improved instruments, such as echelle spectrographs, employing 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 derivatives 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 unparalleled quality and distance range. As often happens in astrophysics the challenge is now coming from the observers to the theorists to provide interpretational tools which are adequate to the state of the data Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Astrophysik (DE-588)4003326-0 gnd rswk-swf Spektrallinie (DE-588)4182165-8 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1984 Triest gnd-content Astrophysik (DE-588)4003326-0 s Spektrallinie (DE-588)4182165-8 s 2\p DE-604 Crivellari, Lucio edt NATO ASI Series, Series C Mathematical and Physical Sciences 152 (DE-604)BV000902768 152 https://doi.org/10.1007/978-94-009-5372-7 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Progress in Stellar Spectral Line Formation Theory Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Astrophysik (DE-588)4003326-0 gnd Spektrallinie (DE-588)4182165-8 gnd |
| subject_GND | (DE-588)4003326-0 (DE-588)4182165-8 (DE-588)1071861417 |
| title | Progress in Stellar Spectral Line Formation Theory |
| title_alt | Proceedings of the NATO Advanced Research Workshop, Grignano-Miramare, Trieste, Italy, September 4-7, 1984 |
| title_auth | Progress in Stellar Spectral Line Formation Theory |
| title_exact_search | Progress in Stellar Spectral Line Formation Theory |
| title_full | Progress in Stellar Spectral Line Formation Theory edited by John E. Beckman, Lucio Crivellari |
| title_fullStr | Progress in Stellar Spectral Line Formation Theory edited by John E. Beckman, Lucio Crivellari |
| title_full_unstemmed | Progress in Stellar Spectral Line Formation Theory edited by John E. Beckman, Lucio Crivellari |
| title_short | Progress in Stellar Spectral Line Formation Theory |
| title_sort | progress in stellar spectral line formation theory |
| topic | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Astrophysik (DE-588)4003326-0 gnd Spektrallinie (DE-588)4182165-8 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Astronomy, Observations and Techniques Astrophysik Spektrallinie Konferenzschrift 1984 Triest |
| url | https://doi.org/10.1007/978-94-009-5372-7 |
| volume_link | (DE-604)BV000902768 |
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