书籍详情
行星状星云概论（英文）
作者：[加] 杰森·J.西山（Jason J.Nishiyama） 著
出版社：哈尔滨工业大学出版社
出版时间：2020-10-01
ISBN：9787560391090
定价：¥38.00
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内容简介
在《行星状星云概论（英文）》中，作者将研究行星状星云是什么，它们从哪里来，又将去向哪里。作者将讨论是什么机制导致了这些恒星消亡的美丽标记，以及是什么导致它们形成了各种各样的形状。《行星状星云概论（英文）》作者还将探讨如何测量行星状星云的各个方面，例如其组成。尽管作者将对行星状星云进行某些方面的数学处理，但主要观点应该是那些只有有限的数学背景的让人容易理解的内容。《行星状星云概论（英文）》的结尾部分附有一些简短的词汇表，在每章的末尾都包含了一个广泛的参考书目，作者特别鼓励有兴趣的读者更深入地了解这些文章。
作者简介
杰森·J.西山（Jason J.Nishiyama），加拿大卡尔加里莱斯布里奇大学的讲师，也是加拿大皇家天文学会卡尔加里中心Wilson Coulee天文台的主任，拥有澳大利亚墨尔本的斯威本科技大学的天文学硕士学位。
目录
Preface
Acknowledgements
Author biography
1 Introduction
1．1 Planetary nebulae
1．2 Discovery and history
1．2．1 Initial discovery
1．2．2 Naming
1．2．3 The road to understanding
1．2．4 Origins and fate revealed
1．2．5 Methods of discovery
1．3 Components of planetary nebulae
1．3．1 Nebular envelope
1．3．2 Central star
References
2 Formation of planetary nebulae
2．1 Planetary nebulae as a stage in stellar evolution
2．1．1 Hertzsprung-Russell diagram
2．1．2 Stellar evolution——main sequence to the AGB
2．1．3 Evolution to the asymptotic giant branch
2．1．4 The asymptotic giant branch
2．1．5 Mass loss
2．2 Proto-planetary nebulae
2．2．1 Morphology
2．3 Progenitor masses
2．3．1 Calculation of white dwarf mass
2．3．2 Calculation of progenitor mass
2．3．3 Fate outside of the bounds
2．4 Post-planetary nebula
2．4．1 White dwarf physical characteristics
2．4．2 White dwarf observational and chemical characteristics
2．5 Interacting stellar winds
2．5．1 The model
2．5．2 Limitations of the model
References
3 Observational data of planetary nebulae
3．1 Chemical abundance
3．1．1 Observed abundance
3．1．2 Galactic chemical gradient
3．1．3 Galactic chemical enrichment
3．2 Distance determination
3．2．1 Difficulties in determining distance
3．2．2 Techniques for determining distance
References
4 Planetary nebula morphology
4．1 Classifying planetary nebulae
4．1．1 Chemical classification
4．1．2 Morphological classification
4．2 Morphology， classification and planetary nebulae evolution
4．2．1 Morphology and planetary nebulae abundance
4．2．2 Morphology and progenitor star mass
4．3 Explaining morphology
4．3．1 Round morphology
4．3．2 Elliptical morphology
4．3．3 Bipolar morphology
4．3．4 Point symmetric morphology
4．4 Concluding remarks
References
Glossary
Symbols
编辑手记
Acknowledgements
Author biography
1 Introduction
1．1 Planetary nebulae
1．2 Discovery and history
1．2．1 Initial discovery
1．2．2 Naming
1．2．3 The road to understanding
1．2．4 Origins and fate revealed
1．2．5 Methods of discovery
1．3 Components of planetary nebulae
1．3．1 Nebular envelope
1．3．2 Central star
References
2 Formation of planetary nebulae
2．1 Planetary nebulae as a stage in stellar evolution
2．1．1 Hertzsprung-Russell diagram
2．1．2 Stellar evolution——main sequence to the AGB
2．1．3 Evolution to the asymptotic giant branch
2．1．4 The asymptotic giant branch
2．1．5 Mass loss
2．2 Proto-planetary nebulae
2．2．1 Morphology
2．3 Progenitor masses
2．3．1 Calculation of white dwarf mass
2．3．2 Calculation of progenitor mass
2．3．3 Fate outside of the bounds
2．4 Post-planetary nebula
2．4．1 White dwarf physical characteristics
2．4．2 White dwarf observational and chemical characteristics
2．5 Interacting stellar winds
2．5．1 The model
2．5．2 Limitations of the model
References
3 Observational data of planetary nebulae
3．1 Chemical abundance
3．1．1 Observed abundance
3．1．2 Galactic chemical gradient
3．1．3 Galactic chemical enrichment
3．2 Distance determination
3．2．1 Difficulties in determining distance
3．2．2 Techniques for determining distance
References
4 Planetary nebula morphology
4．1 Classifying planetary nebulae
4．1．1 Chemical classification
4．1．2 Morphological classification
4．2 Morphology， classification and planetary nebulae evolution
4．2．1 Morphology and planetary nebulae abundance
4．2．2 Morphology and progenitor star mass
4．3 Explaining morphology
4．3．1 Round morphology
4．3．2 Elliptical morphology
4．3．3 Bipolar morphology
4．3．4 Point symmetric morphology
4．4 Concluding remarks
References
Glossary
Symbols
编辑手记
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