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Titlebook: Interstellar Gas Dynamics; H. J. Habing Book 1970 International Astronomical Union 1970 Galaxy.cosmic ray.solar wind.stellar.universe

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樓主: fumble
41#
發(fā)表于 2025-3-28 18:13:56 | 只看該作者
42#
發(fā)表于 2025-3-28 20:49:32 | 只看該作者
43#
發(fā)表于 2025-3-28 23:49:03 | 只看該作者
44#
發(fā)表于 2025-3-29 03:55:45 | 只看該作者
45#
發(fā)表于 2025-3-29 10:43:27 | 只看該作者
Discussion Following the Reports by Parker and Verschuurction 4 is the outcome of another meeting (on September 17). One very extensive remark has been condensed. The latter part of the discussion on September 12 dealt with the informal meeting on HI gas and is presented separately as Chapter 6.
46#
發(fā)表于 2025-3-29 12:49:24 | 只看該作者
47#
發(fā)表于 2025-3-29 19:15:52 | 只看該作者
Supernovae and the Interstellar Medium ambiguous. About all that is certain is that in the supernova event much of the matter is ejected at speeds of typically 10 000 km sec. and that about 10. erg of visible light is emitted. The amount of matter ejected and the bolometric correction to be applied to the optical radiation are very unce
48#
發(fā)表于 2025-3-29 20:13:09 | 只看該作者
The Solar Wind — An Example of a Cosmical Plasma and a Stellar Wind has been worked out by Deutsch (1958, 1960, 1961, 1969) and by Weymann (1960, 1963), who discussed coronal evaporation as a possible mechanism for mass loss in red giants and used hydrodynamical equations for describing the phenomena. During the last few years detailed observations of the solar win
49#
發(fā)表于 2025-3-30 03:31:09 | 只看該作者
ten Lasten Kraft und Moment werden die beiden eigenst?ndigen Bilanzen der Kr?fte und Momente im Fall des Gleichgewichts eines K?rpers und beliebiger Teile desselben postuliert. Diese haupts?chlich von Euler vorgenommene Erg?nzung der Newtonschen Mechanik er?ffnet einen Weg, der die weiterführenden T
50#
發(fā)表于 2025-3-30 05:00:29 | 只看該作者
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