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Die Bestimmung der Dichte des interstellaren Gases aus 21-cm-Beobachtungen (German, Paperback, 1966 ed.) Loot Price: R1,658
Discovery Miles 16 580
Die Bestimmung der Dichte des interstellaren Gases aus 21-cm-Beobachtungen (German, Paperback, 1966 ed.): Kristen Rohlfs

Die Bestimmung der Dichte des interstellaren Gases aus 21-cm-Beobachtungen (German, Paperback, 1966 ed.)

Kristen Rohlfs

Series: Forschungsberichte des Landes Nordrhein-Westfalen, 1704

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Einleitung und Inhaltsi.ibersicht . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 1. Die Struktur und Geschwindigkeitsverteilung der interstellaren Materi- eine Ubersicht . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11 . . . . . . . . . . . . . . . . 2. Der Zusammenhang der Intensitat der 21-cm-Linie mit Dichte und Temperatur des interstellaren Mediums . . . . . . . . . . . . . . . . . . . . 19 . . . . . . . . 3. Die V erteilungsfunktion der kinetischen Wolkentemperaturen . . . . . . . 23 . A. Die V erteilung der StoBzeiten . . . . . . . . . . . . . . . . . . . . . . . 24 . . . . . . . . . . B. Die Abki.ihlungsfunktion des interstellaren Gases . . . . . . . . . . . . . 29 . . . . C. Die Verteilung der Wolkentemperaturen . . . . . . . . . . . . . . . . . 31 . . . . . . . 4. Dichtebestimmung bei endlichem Winkelauflosungsvermogen . . . . . . . 35 . . 5. Wolkenstruktur und Dichtebestimmung . . . . . . . . . . . . . . . . . . . . 40 . . . . . . . . 6. Ein Poisson-Modell der Wolkenverteilung 43 Literaturverzeichnis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49 . . . . . . . . . . . . . . . 5 Summary One of the main tasks of 21-cm investigations consists in the determination of the density of interstellar Hydrogen gas. This has usually been done with the assumption that the Hydrogen gas forms a stratum of more or less uniform density. If Hydrogen clouds exist, they were believed to be transparent for the 21-cm radiation, and the density gradients were supposed to be small. However, in the last years observations accumulated which indicate this picture to be incorrect. The interstellar material seems to be concentrated in clouds of rather high density and considerable opacity but of small diameter. The kinetic temperatures of these clouds need not to be the same for all clouds, in the contrary, rather large temperature variations are indicated. These facts make it necessary to reconsider the derivation of the formulae connecting the measured intensity of the 21-cm radiation with the density of the Hydrogen gas and the kinetic temperature. This paper intends to lead to an improvement for the solution of this problem.

General

Imprint: VS Verlag fur Sozialwissenschaften
Country of origin: Germany
Series: Forschungsberichte des Landes Nordrhein-Westfalen, 1704
Release date: 1966
First published: 1966
Authors: Kristen Rohlfs
Dimensions: 244 x 170 x 3mm (L x W x T)
Format: Paperback
Pages: 54
Edition: 1966 ed.
ISBN-13: 978-3-663-06073-4
Languages: German
Categories: Books > Reference & Interdisciplinary > Encyclopaedias & reference works > General
Books > Science & Mathematics > Science: general issues > General
Books > Children's & Educational > Science > General
Books > Children's Fiction & Fun
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LSN: 3-663-06073-X
Barcode: 9783663060734

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