Showing papers by "Alan Fitzsimmons published in 1990"
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TL;DR: In this paper, high-resolution echelle spectra of a main-sequence B type star (AV 304) in the Small Magellanic Cloud were analyzed using model atmosphere techniques to derive its atmospheric parameters and chemical composition.
Abstract: High-resolution echelle spectra of a main-sequence B type star (AV 304) in the Small Magellanic Cloud are analyzed using model atmosphere techniques to derive its atmospheric parameters and chemical composition. Because AV 340 is at an early evolutionary stage, its chemical composition should reflect that of its progenitor interstellar material. A general heavy element depletion of approximately -0.6 to -0.8 dex is deduced with nitrogen being more severely depleted and oxygen possibly less depleted. Helium has an approximately normal abundance. The high quality of the observational data coupled with the very small projected rotational velocity implies that depletions should normally be accurate to better than + or - 0.2 dex, with the oxygen abundance probably being accurate to + or - 0.1 dex. 43 refs.
17 citations
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TL;DR: Les observations photometriques de la comete de Halley au post-perihelion, du 7 au 10 decembre 1985, sont presentees as discussed by the authors, les taux de production et les largeurs d'echelle des molecules OH and H 2 O du noyau sont determinees.
Abstract: Les observations photometriques de la comete de Halley au post-perihelion , du 7 au 10 decembre 1985, sont presentees. Les taux de production et les largeurs d'echelle des molecules OH et H 2 O du noyau sont determinees.
4 citations
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TL;DR: Les spectres de 6 asteroides, 624 Hektor, 153 Hilda, 279 Thule, 334 Chicago, 1269 Rollandia and 1167 Dubiago, sont presentes as mentioned in this paper.
Abstract: Les spectres de 6 asteroides, 624 Hektor, 153 Hilda, 279 Thule, 334 Chicago, 1269 Rollandia et 1167 Dubiago, sont presentes. Des caracteristiques d'absorption sont determinees dans les spectres de facteur de reflexion de 1269 Rollandia et 279 Thule.
1 citations
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TL;DR: Les observations spectroscopiques des amas doubles h and χ Per et de l'association lointaine Cep OB III sont presentees as mentioned in this paper. And les largeurs equivalentes, les profils de raies et les abondances (calculees avec un modele d'atmosphere ETL) des etoiles (proches) de la sequence principale sont determines.
Abstract: Les observations spectroscopiques des amas doubles h et χ Per et de l'association lointaine Cep OB III sont presentees. Les largeurs equivalentes, les profils de raies et les abondances (calculees avec un modele d'atmosphere ETL) des etoiles (proches) de la sequence principale sont determines.
1 citations