浮华 发表于 2025-3-21 19:35:24

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Basal-Ganglia 发表于 2025-3-21 23:32:02

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ASTER 发表于 2025-3-22 01:55:10

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退潮 发表于 2025-3-22 05:08:04

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乐意 发表于 2025-3-22 09:18:09

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TIA742 发表于 2025-3-22 13:55:09

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刺耳的声音 发表于 2025-3-22 18:35:24

https://doi.org/10.1007/978-94-009-5428-1LOPES; Variation; astronomy; gravity; interferometry; optical interferometry; photometry; planet; radio astr

认为 发表于 2025-3-22 21:46:36

Mass Loss from Red Giants: Results from Ultraviolet Spectroscopy,on lines, such as the Mg II resonance lines, and from Ρ Cygni profile lines of atoms in the dominant ionization stage when a hot star is available to probe the wind of a red giant. The ζ Aur systems, consisting of a K-M supergiant and a main sequence Β star are important systems for which reliable m

形状 发表于 2025-3-23 02:14:03

Thermal Radio Emission from Molecules in Circumstellar Outflows,r. Carbon monoxide emission, now seen in > 100 stars, is a useful probe of the mass loss rate, and the surveys that have been made are beginning to provide an idea of the total rate of return of enriched stellar material to the interstellar medium and give an indication of which objects contribute s

exigent 发表于 2025-3-23 07:21:15

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查看完整版本: Titlebook: Mass Loss from Red Giants; Proceedings of a Con Mark Morris,Ben Zuckerman Conference proceedings 1985 D. Reidel Publishing Company, Dordrec