Non-LTE model atmospheres of hot central stars close to the Eddington limit. The Zanstra discrepancy and the occurence of an emission edge at 228 Å
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 1984, Vol.134 (1), p.139-146 |
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container_title | Astronomy and astrophysics (Berlin) |
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creator | HUSFELD, D KUDRITZKI, R. P SIMON, K. P CLEGG, R. E. S |
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The Zanstra discrepancy and the occurence of an emission edge at 228 Å</title><title>Astronomy and astrophysics (Berlin)</title><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Stars</subject><subject>Stellar atmospheres (photospheres, chromospheres, coronae, magnetospheres). Radiative transfer. 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ispartof | Astronomy and astrophysics (Berlin), 1984, Vol.134 (1), p.139-146 |
issn | 0004-6361 1432-0746 |
language | eng |
recordid | cdi_pascalfrancis_primary_9525144 |
source | EDP Sciences; EZB-FREE-00999 freely available EZB journals |
subjects | Astronomy Earth, ocean, space Exact sciences and technology Stars Stellar atmospheres (photospheres, chromospheres, coronae, magnetospheres). Radiative transfer. Opacity and line formation Stellar characteristics and properties |
title | Non-LTE model atmospheres of hot central stars close to the Eddington limit. The Zanstra discrepancy and the occurence of an emission edge at 228 Å |
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