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Titlebook: Reviews in Modern Astronomy 2; Gerhard Klare Conference proceedings 1989 Springer-Verlag Berlin Heidelberg 1989 Accretion.LOPES.Redshift.S

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樓主: Sinuate
41#
發(fā)表于 2025-3-28 15:40:53 | 只看該作者
42#
發(fā)表于 2025-3-28 21:55:46 | 只看該作者
43#
發(fā)表于 2025-3-28 23:05:01 | 只看該作者
44#
發(fā)表于 2025-3-29 05:38:13 | 只看該作者
45#
發(fā)表于 2025-3-29 07:29:40 | 只看該作者
46#
發(fā)表于 2025-3-29 14:10:15 | 只看該作者
Synchrotron Light from Extragalactic Radio Jets and Hot Spots,rared and optical wavelengths. Detailed maps of the optical spectral index in the jets of M 87 and 3C 273 do not show the pronounced variations predicted by standard acceleration models (. shock acceleration).
47#
發(fā)表于 2025-3-29 16:59:48 | 只看該作者
Very High Energy X-Rays from Supernova 1987A,e the bolometric light curve, the detection of infrared and gamma-ray line radiation and the detection of the very high energy X-ray continuum, all connected to the existence and spatial distribution of 0.075 M. of radioactive .Co in the debris of this stellar collaps.
48#
發(fā)表于 2025-3-29 22:59:43 | 只看該作者
Astrophysics with GRO,bservatories (The Advanced X-Ray Astrophysics Facility: AXAF, and the Space Infrared Telescope Facility: SIRTF) both are still in the planning phase. The four Great Observatories will cover the electromagnetic spectrum from infrared to gamma-ray energies and will lead to an enormous progress in space astronomy.
49#
發(fā)表于 2025-3-30 03:50:56 | 只看該作者
The Muenster Redshift Project (MRSP),troduce systematic errors into the derivation of global quantities (galaxy correlation functions, mean galaxy density, luminosity function .) and of cosmological parameters (Hubble constant, deceleration parameter, density parameter, cosmological constant).
50#
發(fā)表于 2025-3-30 06:47:56 | 只看該作者
Atmospheric Variations in Chemically Peculiar Stars,f CP stars. This paper deals exclusively with the classical Ap stars, stars in the spectral range from F to B that show magnetic fields, the CP2 stars in Prestons notation. In these stars we have the possibility to study the interaction of a stellar photosphere with a strong, large scale magnetic field.
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