Titlebook: Dusty Objects in the Universe; Proceedings of the F E. Bussoletti,A. A. Vittone Conference proceedings 1990 Kluwer Academic Publishers 1990

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Conference proceedings 1990tical interpretations which concern processes occurring in our Galaxy and in external galaxies. The Workshop gave to participants the unique opportunity of exchanging ideas and of discussing on different themes. In addition, the meeting has been enriched by the presentation of the major technologica

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0067-0057 opportunity of exchanging ideas and of discussing on different themes. In addition, the meeting has been enriched by the presentation of the major technologica978-94-010-6782-9978-94-009-0661-7Series ISSN 0067-0057 Series E-ISSN 2214-7985

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On the possible interaction between magnetic field and HII region in AB Aurellar wind in the line-forming region, we observe an emission component in the blue side of the absorption feature (Beals Type III profile). Furthermore, the combined effects of the oblique rotator geometry and the mass loss produced by the centrifugal force give rise to the changing Type II P Cyg p

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When Will a Repost Cascade Settle Down?anic materials. Those results have been reviewed in recent literature with a view to their astrophysical relevance (e.g. Strazzulla and Johnson 1989, Andronico et al. 1987, Lanzerotti et al. 1987, Foti et al. 1984, Johnson et al. 1984).

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Thanh Trinh,Dingming Wu,Joshua Zhexue Huangypes of astronomical objects (reviewed by Allamandola, 1984; Willner, 1984; Léger and d’Hendecourt, 1987; Mamandola, Tielens, and Barker, 1987). It has been postulated that these features may arise from aromatic hydrocarbons (Duley and Williams, 1981; Léger and Puget, 1984; Allamandola, Tielens and

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Yan Zhuang,Guoliang Li,Jianhua Fenge, the simplest polycyclic aromatic hydrocarbon molecule. Naphthalene is observed to attach to Si. and to alter its chemistry. The observed gas-phase reactions of the Si..naphthalene adduct are viewed as “surface reactions”. They provide a novel route for the synthesis of Si-bearing molecules. The r

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Rukshan Alexander,David Murray,Nik Thompsonlected temperatures. Changes in the aborbance spectum at elevated temperatures include a 3—fold strengthening of coronene’s 3.29 .m band which assumes a profile very similar to the 3.29 .m UIR band. Coronene’s 8.8 .m feature which is also correlated with a UIR also shows substantial increases in int