Emg827 发表于 2025-3-27 00:42:41
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Interstellar Matter, Nebulae,the presence of an interesting correlation between the gas and dust in this region. A dust filament is shown to run parallel to, but displaced towards the galactic plane from, a ridge of enhanced H I emission. It is suggested that this results from the passage of a shock wave through the system, res自由职业者 发表于 2025-3-27 08:06:48
Radio Sources, X-ray Sources, Cosmic Radiation, polarization burst during which the 2.2 µm polarization rose from 17.5 to 28.7 per cent and fell again to 14.9 per cent. At its peak the degree of optical polarization was 43.9 per cent. The data show the degree of polarization to increase towards shorter wavelengths. The large changes in polarizat营养 发表于 2025-3-27 11:19:42
Stellar Systems, Galaxy, Extragalactic Objects, Cosmology,ly 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.新陈代谢 发表于 2025-3-27 17:39:23
Book 1982tains 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锯齿状 发表于 2025-3-27 18:36:52
0067-0022 d in earlier volumes is also included. We acknowledge with thanks contributions to this volume by Dr. J. Bouska, Prague, who surveyed journals and publications 978-3-662-12336-2978-3-662-12334-8Series ISSN 0067-0022整体 发表于 2025-3-27 22:30:36
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Sun,ning of the lower photospheric temperature gradient, corresponding to a 15% increase in mixing length, at constant, effective temperature. The associated increase in the efficiency of convection can be reconciled with a constant luminosity if the change is assumed to occur only in the outer ~ 100 km of the convection zone.Commonwealth 发表于 2025-3-28 09:40:33
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