  Vibrational stability of G plus modes towards non-radial oscillations for solar modelsNoels-Grötsch, Arlette  ; Gabriel, Maurice ; et alin Mémoires de la Societe Royale des Sciences de Liège (1975), 8 The vibrational stability of solar models towards g plus modes has been studied from the Zero Age Main Sequence (ZAMS) up to the age of 5 billion yr. The nuclear energy contribution to instability is ... [more ▼] The vibrational stability of solar models towards g plus modes has been studied from the Zero Age Main Sequence (ZAMS) up to the age of 5 billion yr. The nuclear energy contribution to instability is calculated with the effective sensitivity of the reactions to change of temperature. The perturbation of convective terms is taken from an extension for nonradial oscillations of Unno's theory. The ZAMS model and the present sun are stable. However, for intermediate ages, models are unstable with respect to the lowest modes due to the effects of nuclear reactions. If, moreover, the mechanical effects of convection are taken into account, all models are unstable. However their theory is uncertain enough to require caution. [less ▲] Detailed reference viewed: 6 (0 ULg)Phénomènes de fluorescence dans les astres.Swings, Polydore in Mémoires de la Societe Royale des Sciences de Liège (1971), 1 Detailed reference viewed: 7 (2 ULg)Free radicals in astrophysics.Swings, Polydore in Mémoires de la Societe Royale des Sciences de Liège (1969), XVIII(3), 7-26 Detailed reference viewed: 5 (1 ULg)Consideration of the forbidden lines of iron in the states from Fe0 to Fe6+Swings, Polydore ; Swings, Jean-Pierre in Mémoires de la Societe Royale des Sciences de Liège (1969), 17 The iron atom which has a fairly high cosmic abundance presents the great interest of appearing in a wide variety of stars and nebulae, at many stages of ionization, and of revealing forbidden transitions ... [more ▼] The iron atom which has a fairly high cosmic abundance presents the great interest of appearing in a wide variety of stars and nebulae, at many stages of ionization, and of revealing forbidden transitions in emission in many of these ionization stages. The present paper discusses the following topics : (a) the case of the as yet undiscovered forbidden lines of neutral iron (Fe0) ; (b) some recently acquired astronomical information on the forbidden lines of the stages Fe+ to Fe6+ ; (c) general considerations on the important information revealed by these forbidden lines of iron on the physical structure and excitation mechanisms which are present in the emission line stars of early and late types. For lack of time we give only a very summarized version of our paper ; a complete text will appear later. [less ▲] Detailed reference viewed: 7 (4 ULg)Considérations relatives à la distribution des conditions physiques au sein des atmosphères stellairesSwings, Polydore in Mémoires de la Societe Royale des Sciences de Liège (1938), III Detailed reference viewed: 9 (6 ULg)Sur la probabilité de désactivation par chocs intermoléculaires, dans le cas des émissions fluorescentesSwings, Polydore in Mémoires de la Societe Royale des Sciences de Liège (1931), XVI Detailed reference viewed: 10 (8 ULg)Note sur un procédé simple permettant l'étude en laboratoire, des méthodes de photométrie stellaire photographiqueSwings, Polydore ; in Mémoires de la Societe Royale des Sciences de Liège (1930), XV Detailed reference viewed: 5 (2 ULg)Attraction d'un corps formé de couches sphériques concentriques homogènes, sur un point extérieur, dans le cas d'un potentiel riemannien : applications des potentiels rimanniens au cas d'un corps sphériqueSwings, Polydore in Mémoires de la Societe Royale des Sciences de Liège (1928), XIV Detailed reference viewed: 9 (2 ULg) |
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