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A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph

2008 doctoral thesis by Siramas Komonjinda at University of Canterbury
Place doctoral_thesis Q112877695
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A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph

Summary

A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph is a doctoral thesis[1].

Key Facts

  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph authored Siramas Komonjinda[2].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's instance of is recorded as doctoral thesis[3].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's publisher is recorded as UC Research Repository[4].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's DOI is recorded as 10.26021/5921[5].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's language of work or name is recorded as English[6].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's country of origin is recorded as New Zealand[7].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's publication date is recorded as +2008-00-00T00:00:00Z[8].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's work available at URL is recorded as https://ir.canterbury.ac.nz/handle/10092/1590[9].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's Handle ID is recorded as 10092/1590[10].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's title is recorded as A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph[11].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's copyright holder is recorded as Siramas Komonjinda[12].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's thesis submitted to is recorded as University of Canterbury[13].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's on focus list of Wikimedia project is recorded as NZThesisProject[14].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's copyright status is recorded as copyrighted[15].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's online access status is recorded as open access[16].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's thesis committee member is recorded as John B. Hearnshaw[17].
  • A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph's thesis committee member is recorded as David John Ramm[18].

Body

Designation and Status

A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph'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] ↑ . 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] ↑ . astrogen.aas.org. astrogen.aas.org. Provenance: wikidata.org.
  17. [18] ↑ . 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). A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph. Retrieved May 3, 2026, from https://4ort.xyz/entity/a-study-of-binary-star-orbits-using-precise-radial-velocity-measurements-with-the-hercules-spectrograph
MLA “A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/a-study-of-binary-star-orbits-using-precise-radial-velocity-measurements-with-the-hercules-spectrograph.
BibTeX @misc{4ortxyz_a-study-of-binary-star-orbits-using-precise-radial-velocity-measurements-with-the-hercules-spectrograph_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph}}, year = {2026}, url = {https://4ort.xyz/entity/a-study-of-binary-star-orbits-using-precise-radial-velocity-measurements-with-the-hercules-spectrograph}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): A study of binary star orbits using precise radial velocity measurements with the HERCULES spectrograph — https://4ort.xyz/entity/a-study-of-binary-star-orbits-using-precise-radial-velocity-measurements-with-the-hercules-spectrograph (retrieved 2026-05-03)

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