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On the evolutionary status of J stars
2008 (English)Independent thesis Advanced level (professional degree), 20 credits / 30 HE creditsStudent thesis
Abstract [en]

This research, which is an MSc diploma work in engineering physics at LuleƄ University of Technology, investigates the properties and possible origins of the J-type carbon stars. In particular, it shows that R stars are almost certainly progenitors of some, but not all, J stars. It also shows that the evolution of an intermediate mass AGB star can produce properties seen in J stars, albeit for a short time only. This research concludes that the J stars come from more than one kind of progenitor star, and that a full explanation is still lacking. This research was undertaken at Monash University in Melbourne (Australia) as part of the exchange programme between the two universities.

Place, publisher, year, edition, pages
2008.
Keyword [en]
Physics Chemistry Maths, Astronomy
Keyword [sv]
Fysik, Kemi, Matematik
Identifiers
URN: urn:nbn:se:ltu:diva-55628ISRN: LTU-EX--08/120--SELocal ID: c789c65c-8434-4b10-bc10-51d1d49b7230OAI: oai:DiVA.org:ltu-55628DiVA: diva2:1029012
Subject / course
Student thesis, at least 30 credits
Educational program
Engineering Physics, master's level
Examiners
Note
Validerat; 20101217 (root)Available from: 2016-10-04 Created: 2016-10-04Bibliographically approved

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CiteExportLink to record
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Citation style
  • apa
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  • de-DE
  • en-GB
  • en-US
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Output format
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