Dignant
发表于 2025-3-26 23:52:01
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outset
发表于 2025-3-27 04:57:01
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运动性
发表于 2025-3-27 07:25:14
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痛得哭了
发表于 2025-3-27 09:55:04
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Recess
发表于 2025-3-27 17:20:17
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低三下四之人
发表于 2025-3-27 18:29:47
Changes in Interstellar Atomic Abundances from the Galactic Plane to the Halo,not seem to change appreciably. A likely explanation for the apparent increase of iron is the partial sputtering of material off the surfaces of dust grains by interstellar shocks. Another possibility might be that the ejecta from type I supernovae enrich the low density medium in the halo with iron.
Instinctive
发表于 2025-3-28 00:51:29
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苦涩
发表于 2025-3-28 03:34:00
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enumaerate
发表于 2025-3-28 10:09:58
On the Analysis of Motions Perpendicular to the Galactic Plane,one has succeeded in deriving a valid curve of the acceleration ..; typically the curve turns over in a way that implies negative densities at some distance from the galactic plane. What I would like to do in this brief note is to suggest some possible reasons for this difficulty--specifically, that the types of stars used have been unsuitable.
束以马具
发表于 2025-3-28 11:03:24
0067-0057 d at Penticton in June 1981. Leo Blitz (now at the University of Maryland) and I decided that there was a need, and agreed that we would organize one in Vancouver in the Spring of 1982. The purpose of the workshop was to have an intensive exchange of ideas between some of the most active workers in