blithe
发表于 2025-3-25 06:23:26
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arabesque
发表于 2025-3-25 10:03:16
978-3-662-13647-8Springer-Verlag Berlin Heidelberg 1988
Champion
发表于 2025-3-25 13:12:18
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flourish
发表于 2025-3-25 16:57:57
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champaign
发表于 2025-3-25 22:19:15
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有偏见
发表于 2025-3-26 03:27:51
Interpretation difficulties of SNR shock spectra,ough shock parameters such as velocity and preshock density are significantly different. If the shocks are radiatively unstable, then it may be possible to observe time variations of line ratios in SNRs over a period of a few years.
Spinal-Tap
发表于 2025-3-26 07:02:15
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gnarled
发表于 2025-3-26 11:29:19
Kinematics of optical filaments in the Cygnus Loop,. In both lines a number of different components contributing to the emission are recognized. The emission indicates that the gas may lie in a thin sheet, while from the Hα emission this indication is much less clear.
发出眩目光芒
发表于 2025-3-26 15:21:37
W. Reich,E. Fürst These sets are higher-degree analogs of the corresponding sets under the angle-doubling map of the circle, which played a key role in Douady and Hubbard‘s work on the quadratic family and the Mandelbrot set. Presenting the first systematic study of rotation sets, treating both rational and irration
Feedback
发表于 2025-3-26 18:06:40
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