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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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發(fā)表于 2025-3-21 17:11:27 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Dusty Objects in the Universe
副標(biāo)題Proceedings of the F
編輯E. Bussoletti,A. A. Vittone
視頻videohttp://file.papertrans.cn/284/283451/283451.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Dusty Objects in the Universe; Proceedings of the F E. Bussoletti,A. A. Vittone Conference proceedings 1990 Kluwer Academic Publishers 1990
描述Solid matter in space is crucial in accounting for many processes. In these last years a great improvement of the general knowledge of the problem has been possible due to the increase, in number and quality, of observations and of the laboratory efforts to simulate "cosmic" dust. Theoreticians have also given their contribution in solving some questions and in posing others. Continuing an effort started in 1987, the Astrophysical Groups operating in Naples th th have considered it useful to organize a Workshop in Capri from September 8 to 13 1989 in order to assess the state of the art in such an interesting field as that of "Dusty Objects in the Universe". The subject is, obviously, too wide to be discussed in detail. However, the presence of many experts in different areas provided an updated general picture. Laboratory work has been reviewed, as well as recent observations and theoretical 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
出版日期Conference proceedings 1990
關(guān)鍵詞Galaxy; astronomy; cosmology; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-0661-7
isbn_softcover978-94-010-6782-9
isbn_ebook978-94-009-0661-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightKluwer Academic Publishers 1990
The information of publication is updating

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0067-0057 roblem has been possible due to the increase, in number and quality, of observations and of the laboratory efforts to simulate "cosmic" dust. Theoreticians have also given their contribution in solving some questions and in posing others. Continuing an effort started in 1987, the Astrophysical Group
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Hendi Lie,Richi Nayak,Gordon Wyeth from the higher spectral resolution and higher sensitivity currently available. Laboratory work on identification of the feature emitting material is abo reviewed, and different candidate materials for the features are compared.
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Astrophysical Implications of the Infrared Spectrum of Coronene at Elevated Temperaturesensity at elevated temperatures. The 10.5 .m feature of coronene which does not correlate with the UIR decreases sharply as the temperature is increased. These results as well as some possible implications are discussed.
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