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010   $a3-540-46971-0
024 7 $a10.1007/BFb0036058
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035   $a(DE-He213)978-3-540-46971-1
035   $a(PPN)155208322
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100   $a20121227d1990      u|             0
101 0 $aeng
135   $aurnn|008mamaa
181   $ctxt
182   $cc
183   $acr
200 10$aAccuracy of Element Abundances from Stellar Atmospheres$b[electronic resource] $eProceedings of Two Sessions Allocated at the IAU General Assembly in Baltimore, USA, August 1988 /$fedited by Rainer Wehrse
205   $a1st ed. 1990.
210  1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d1990.
215   $a1 online resource (V, 109 p. 1 illus.) 
225 1 $aLecture Notes in Physics,$x0075-8450 ;$v356
300   $aBibliographic Level Mode of Issuance: Monograph
311   $a3-540-52365-0 
327   $aOn the accuracy of atomic transition probabilities -- Accuracy of excitation and ionisation cross sections -- Accuracy of line broadening data -- Accuracy of abundances from O to mid B main sequence stars -- The accuracy of abundances from middle B to F main sequence normal stars -- Accuracy of the determination of the abundances in solar type stars -- Problems associated with cool dwarf stars -- Accuracy of abundances from stars in near-by galaxies.
330   $aTo get a reasonably realistic picture of the structure and evolution of stars one needs to know accurately the abundances of chemical elements and their isotopes in the stellar atmosphere and in the galactic environment of the stars. The articles collected in this volume give a modern review of the abundance accuracies for main-sequence stars. After a general introduction in the first part the accuracies of atomic transition probabilities, ionization and excitation cross-sections, and line broad- ening data are discussed. In the second part the specific problems and results for different stellar types are presented, and, finally, an overview on the possibilities of abundance determinations for stars outside the Galaxy is given.
410  0$aLecture Notes in Physics,$x0075-8450 ;$v356
606   $aObservations, Astronomical
606   $aAstronomy?Observations
606   $aAstrophysics
606   $aLasers
606   $aPhotonics
606   $aGeophysics
606   $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014
606   $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022
606   $aOptics, Lasers, Photonics, Optical Devices$3https://scigraph.springernature.com/ontologies/product-market-codes/P31030
606   $aGeophysics/Geodesy$3https://scigraph.springernature.com/ontologies/product-market-codes/G18009
615  0$aObservations, Astronomical.
615  0$aAstronomy?Observations.
615  0$aAstrophysics.
615  0$aLasers.
615  0$aPhotonics.
615  0$aGeophysics.
615 14$aAstronomy, Observations and Techniques.
615 24$aAstrophysics and Astroparticles.
615 24$aOptics, Lasers, Photonics, Optical Devices.
615 24$aGeophysics/Geodesy.
676   $a520
702   $aWehrse$b Rainer$4edt$4http://id.loc.gov/vocabulary/relators/edt
906   $aBOOK
912   $a996466712903316
996   $aAccuracy of Element Abundances from Stellar Atmospheres$92538652
997   $aUNISA