古生物学
发表于 2025-3-21 19:03:32
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补角
发表于 2025-3-21 21:29:49
Preliminaries,lly gives rise to the radiation we see streaming off the surface. The vast majority of stars spend most of their active lives in such an equilibrium state, converting hydrogen into helium, and it is only this gradual transmutation of elements by the fusion process that eventually causes their struct
Receive
发表于 2025-3-22 01:43:22
Asteroseismology,radius, and color variations to probe stellar interiors in much the same spirit as in terrestrial seismology. This is not a new subject but it has blossomed in recent years. A review of the list of variables we gave in Chapter 2 makes it clear that the subject spans all phases of stellar evolution.
Derogate
发表于 2025-3-22 05:26:04
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Creditee
发表于 2025-3-22 09:45:51
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BANAL
发表于 2025-3-22 14:45:15
Structure and Evolution of White Dwarfs, as the endpoint of evolution for most stars. The variable white dwarfs, discussed in the final section, will be shown to play an important role in this program. There is no one text that deals solely with these objects but, for further reading, we suggest (1980), (1983), (1984), (1990), (1990), (1990), (1991), (1992), (2001), (2002), and (2003).
reception
发表于 2025-3-22 17:30:21
0941-7834second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e?ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of,
搜集
发表于 2025-3-22 21:43:00
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沉积物
发表于 2025-3-23 01:39:17
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Incommensurate
发表于 2025-3-23 06:47:18
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