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Titlebook: Cosmic Magnetic Fields; Richard Wielebinski,Rainer Beck Book 2005 Springer-Verlag Berlin Heidelberg 2005 astrophysics.cosmic magnetic fiel

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樓主: Agitated
41#
發(fā)表于 2025-3-28 16:24:24 | 只看該作者
Stellar Magnetic Fields,pre-main sequence and on late- and early-type main sequence stars, with some discussion also of red giants and white dwarfs, and with a brief reference to neutron stars. The current observational situation is reviewed, and some of the consequences for our ideas on star formation, on stellar structur
42#
發(fā)表于 2025-3-28 19:44:06 | 只看該作者
43#
發(fā)表于 2025-3-29 01:41:44 | 只看該作者
Numerical Magnetohydrodynamics in Astrophysics,rithms and computational methods have been developed for simulating the time-evolution of magnetic field configurations in the astrophysical environment. The most recent trends go in the direction of fully conservative schemes and adaptive mesh refinement for large-scale supercomputing. The most pop
44#
發(fā)表于 2025-3-29 03:28:39 | 只看該作者
The Foundations of Postmodernismstars (Mestel, 1990). . distributes energy from supernova explosions within the ISM (Subramanian, 1998) and regenerates the field via . (Wielebinski, R., Krause, 1993, Beck et al., 1996; Sect. 6). . is a possible heating source for the ISM and halo gas (Birk et al., 1998). Magnetic fields also contr
45#
發(fā)表于 2025-3-29 09:51:51 | 只看該作者
Magnetic Fields in Galaxies,stars (Mestel, 1990). . distributes energy from supernova explosions within the ISM (Subramanian, 1998) and regenerates the field via . (Wielebinski, R., Krause, 1993, Beck et al., 1996; Sect. 6). . is a possible heating source for the ISM and halo gas (Birk et al., 1998). Magnetic fields also contr
46#
發(fā)表于 2025-3-29 14:54:13 | 只看該作者
Magnetic Fields in Galaxy Systems, Clusters and Beyond,
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