DUCE 发表于 2025-3-26 21:41:58
Plans for High Resolution Imaging with the VLT,possible. In the past most astronomers have emphasized the light gathering function as is evidenced by the common characterization of telescopes by their diameter. Only in specialized subfields, like solar and planetary astronomy, has the angular resolution been a prime characteristic. In the recentheirloom 发表于 2025-3-27 03:29:48
http://reply.papertrans.cn/83/8295/829473/829473_32.pngellagic-acid 发表于 2025-3-27 08:56:26
The Muenster Redshift Project (MRSP),aynes 1990) do not cover a representative part of the universe. It was found that the small scales reached and the small number of objects observed introduce systematic errors into the derivation of global quantities (galaxy correlation functions, mean galaxy density, luminosity function .) and of c串通 发表于 2025-3-27 09:51:57
http://reply.papertrans.cn/83/8295/829473/829473_34.png终端 发表于 2025-3-27 17:00:43
Synchrotron Light from Extragalactic Radio Jets and Hot Spots, for optical synchrotron emission from the jets of M 87 and 3C 273 as well as from three radio hot spots (3C 20 west, 3C 33 south and Pictor A west). Another five objects are very good candidates for emitting synchrotron light. The relevance of optical synchrotron emission as tracer of . particle acAlpha-Cells 发表于 2025-3-27 17:48:43
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Atmospheric Variations in Chemically Peculiar Stars,n on the upper main sequence. In this volume . (1989) gives a compilation of the variety of photometric and spectroscopic properties of all subtypes of 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