Titlebook: Stellar Interiors; Physical Principles, Carl J. Hansen,Steven D. Kawaler,Virginia Trimble Textbook 2004Latest edition Springer Science+Busi

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書(shū)目名稱(chēng)Stellar Interiors影響因子(影響力)

書(shū)目名稱(chēng)Stellar Interiors影響因子(影響力)學(xué)科排名

書(shū)目名稱(chēng)Stellar Interiors網(wǎng)絡(luò)公開(kāi)度

書(shū)目名稱(chēng)Stellar Interiors網(wǎng)絡(luò)公開(kāi)度學(xué)科排名

書(shū)目名稱(chēng)Stellar Interiors被引頻次

書(shū)目名稱(chēng)Stellar Interiors被引頻次學(xué)科排名

書(shū)目名稱(chēng)Stellar Interiors年度引用

書(shū)目名稱(chēng)Stellar Interiors年度引用學(xué)科排名

書(shū)目名稱(chēng)Stellar Interiors讀者反饋

書(shū)目名稱(chēng)Stellar Interiors讀者反饋學(xué)科排名

只看該作者 · 發(fā)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

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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.

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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).

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0941-7834 second 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,

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