Three case studies in spectroscopic mode identification of non-radially pulsating stars

2011 doctoral thesis by Florian Maisonneuve at University of Canterbury
Place doctoral_thesis Q112887101
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Three case studies in spectroscopic mode identification of non-radially pulsating stars

Summary

Three case studies in spectroscopic mode identification of non-radially pulsating stars is a doctoral thesis[1].

Key Facts

  • Three case studies in spectroscopic mode identification of non-radially pulsating stars authored Florian Maisonneuve[2].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's instance of is recorded as doctoral thesis[3].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's publisher is recorded as UC Research Repository[4].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's DOI is recorded as 10.26021/8902[5].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's language of work or name is recorded as English[6].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's country of origin is recorded as New Zealand[7].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's publication date is recorded as +2011-00-00T00:00:00Z[8].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's main subject is recorded as spectroscopy[9].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's Handle ID is recorded as 10092/5395[10].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's title is recorded as Three case studies in spectroscopic mode identification of non-radially pulsating stars[11].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's copyright holder is recorded as Florian Maisonneuve[12].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's thesis submitted to is recorded as University of Canterbury[13].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's on focus list of Wikimedia project is recorded as NZThesisProject[14].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's copyright status is recorded as copyrighted[15].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's online access status is recorded as open access[16].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's thesis committee member is recorded as Karen Rylvia Pollard[17].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's thesis committee member is recorded as Peter Ledsam Cottrell[18].
  • Three case studies in spectroscopic mode identification of non-radially pulsating stars's thesis committee member is recorded as John B. Hearnshaw[19].

Body

Designation and Status

Three case studies in spectroscopic mode identification of non-radially pulsating stars's instance of is recorded as doctoral thesis[3].

References

Programmatic citations — every numbered marker resolves to a verifiable graph row below.

Direct Wikidata claims

  1. [3] . wikidata.org.
  2. [2] . hdl.handle.net. hdl.handle.net. Provenance: wikidata.org.
  3. [4] . wikidata.org.
  4. [5] . wikidata.org.
  5. [6] . wikidata.org.
  6. [7] . wikidata.org.
  7. [8] . wikidata.org.
  8. [9] . hdl.handle.net. hdl.handle.net. Provenance: wikidata.org.
  9. [10] . wikidata.org.
  10. [11] . wikidata.org.
  11. [12] . wikidata.org.
  12. [13] . wikidata.org.
  13. [14] . wikidata.org.
  14. [15] . wikidata.org.
  15. [16] . wikidata.org.
  16. [17] . wikidata.org.
  17. [18] . astrogen.aas.org. astrogen.aas.org. Provenance: wikidata.org.
  18. [19] . astrogen.aas.org. astrogen.aas.org. Provenance: wikidata.org.

Class ancestry

  1. [1] . Wikidata. wikidata.org.

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APA 4ort.xyz Knowledge Graph. (2026). Three case studies in spectroscopic mode identification of non-radially pulsating stars. Retrieved May 3, 2026, from https://4ort.xyz/entity/three-case-studies-in-spectroscopic-mode-identification-of-non-radially-pulsating-stars
MLA “Three case studies in spectroscopic mode identification of non-radially pulsating stars.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/three-case-studies-in-spectroscopic-mode-identification-of-non-radially-pulsating-stars.
BibTeX @misc{4ortxyz_three-case-studies-in-spectroscopic-mode-identification-of-non-radially-pulsating-stars_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Three case studies in spectroscopic mode identification of non-radially pulsating stars}}, year = {2026}, url = {https://4ort.xyz/entity/three-case-studies-in-spectroscopic-mode-identification-of-non-radially-pulsating-stars}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Three case studies in spectroscopic mode identification of non-radially pulsating stars — https://4ort.xyz/entity/three-case-studies-in-spectroscopic-mode-identification-of-non-radially-pulsating-stars (retrieved 2026-05-03)

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