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An introduction to planetary nebulae /

In this book we will look at what planetary nebulae are, where they come from and where they go. We will discuss what mechanisms cause these beautiful markers of stellar demise as well as what causes them to form their variety of shapes. How we measure various aspects of planetary nebulae such as wh...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Nishiyama, Jason J. (Autor)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: San Rafael [California] (40 Oak Drive, San Rafael, CA, 94903, USA) : Morgan & Claypool Publishers, [2018]
Colección:IOP (Series). Release 4.
IOP concise physics.
Temas:
Acceso en línea:Texto completo

MARC

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020 |z 9781681749570  |q print 
024 7 |a 10.1088/978-1-6817-4960-0  |2 doi 
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082 0 4 |a 523.1135  |2 23 
100 1 |a Nishiyama, Jason J.,  |e author. 
245 1 3 |a An introduction to planetary nebulae /  |c Jason J. Nishiyama. 
264 1 |a San Rafael [California] (40 Oak Drive, San Rafael, CA, 94903, USA) :  |b Morgan & Claypool Publishers,  |c [2018] 
264 2 |a Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) :  |b IOP Publishing,  |c [2018] 
300 |a 1 online resource (various pagings) :  |b illustrations (some color). 
336 |a text  |2 rdacontent 
337 |a electronic  |2 isbdmedia 
338 |a online resource  |2 rdacarrier 
490 1 |a [IOP release 4] 
490 1 |a IOP concise physics,  |x 2053-2571 
500 |a "Version: 20180501"--Title page verso. 
500 |a "A Morgan & Claypool publication as part of IOP Concise Physics"--Title page verso. 
504 |a Includes bibliographical references. 
505 0 |a 1. Introduction -- 1.1. Planetary nebulae -- 1.2. Discovery and history -- 1.3. Components of planetary nebulae 
505 8 |a 2. Formation of planetary nebulae -- 2.1. Planetary nebulae as a stage in stellar evolution -- 2.2. Proto-planetary nebulae -- 2.3. Progenitor masses -- 2.4. Post-planetary nebula -- 2.5. Interacting stellar winds 
505 8 |a 3. Observational data of planetary nebulae -- 3.1. Chemical abundance -- 3.2. Distance determination 
505 8 |a 4. Planetary nebula morphology -- 4.1. Classifying planetary nebulae -- 4.2. Morphology, classification and planetary nebulae evolution -- 4.3. Explaining morphology -- 4.4. Concluding remarks. 
520 3 |a In this book we will look at what planetary nebulae are, where they come from and where they go. We will discuss what mechanisms cause these beautiful markers of stellar demise as well as what causes them to form their variety of shapes. How we measure various aspects of planetary nebulae such as what they are made of will also be explored. Though we will give some aspects of planetary nebulae mathematical treatment, the main points should be accessible to people with only a limited background in mathematics. A short glossary of some of the more arcane astronomical terms is at the end of the book to help in understanding. Included at the end of each chapter is an extensive bibliography to the peer reviewed research on these objects and I would encourage the reader interested in an even deeper understanding to read these articles. 
521 |a Anyone with at least a limited background on mathematics. 
530 |a Also available in print. 
538 |a Mode of access: World Wide Web. 
538 |a System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader. 
545 |a Jason Nishiyama is a Sessional Lecturer with the University of Lethbridge Calgary Campus and is the director of the RASC Calgary Centre's Wilson Coulee Observatory. He received his MSc in Astronomy from the Swinburne University of Technology in Melbourne, Australia. His current research is in planetary nebulae morphology. Jason lives in Calgary, Canada. 
588 0 |a Title from PDF title page (viewed on June 12, 2018). 
650 0 |a Planetary nebulae. 
650 7 |a Physics.  |2 bicssc 
650 7 |a SCIENCE / Physics / General.  |2 bisacsh 
710 2 |a Morgan & Claypool Publishers,  |e publisher. 
710 2 |a Institute of Physics (Great Britain),  |e publisher. 
776 0 8 |i Print version:  |z 9781681749570 
830 0 |a IOP (Series).  |p Release 4. 
830 0 |a IOP concise physics. 
856 4 0 |u https://iopscience.uam.elogim.com/book/978-1-6817-4960-0  |z Texto completo