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Titlebook: Astronomy and Astrophysics Abstracts; Literature 1982, Par S. Böhme,W. Fricke,G. Zech Book 1982 Springer-Verlag Berlin Heidelberg 1982 astr

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期刊全称Astronomy and Astrophysics Abstracts
期刊简称Literature 1982, Par
影响因子2023S. Böhme,W. Fricke,G. Zech
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学科分类Astronomy and Astrophysics Abstracts
图书封面Titlebook: Astronomy and Astrophysics Abstracts; Literature 1982, Par S. Böhme,W. Fricke,G. Zech Book 1982 Springer-Verlag Berlin Heidelberg 1982 astr
影响因子Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is devoted to the recording, summarizing and indexing of astronomical publications throughout the world. It is prepared under the auspices of the International Astronomical Union (according to a resolution adopted at the 14th General Assembly in 1970). Astronomy and Astrophysics Abstracts aims to present a comprehensive documenta­ tion of literature in all fields of astronomy and astrophysics. Every effort will be made to ensure that the average time interval between the date of receipt of the original literature and publication of the abstracts will not exceed eight months. This time interval is near to that achieved by monthly abstracting journals, compared to which our system of accumu­ lating abstracts for about six months offers the advantage of greater convenience for the user. Volume 31 contains literature published in 1982 and received before July 15, 1982; some older literature which was received late and which is not recorded in earlier volumes is also included. We acknowledge with thanks contributions to this volume by Dr. J. Bouska, Prague, who surveyed journals and publications
Pindex Book 1982
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https://doi.org/10.1007/978-3-7091-8815-6ly different situations are possible, in two of these the gas layer is warped. The morphology of elliptical radio galaxies with dust lanes such as NGC 5128 (Cen A) and M 84 can be understood on the basis of this model; transient phenomena are not required.
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Pigments of Fungi (Macromycetes),eselected random samples with insufficient knowledge of the data, e.g. from intensity measurements with definite flux density results as well as upper limits. The information contained in inconclusive or inexact results is fully used.
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