Q88926733

spectroscopic binary in the constellation Dorado
Thing spectroscopic_binary Q88926733
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Q88926733

Summary

Q88926733 is a spectroscopic binary[1].

Key Facts

  • Q88926733's instance of is recorded as spectroscopic binary[2].
  • Q88926733's constellation is recorded as Dorado[3].
  • Q88926733's spectral class is recorded as O9.7IV:(n)+sec:[4].
  • Q88926733's spectral class is recorded as O9.7 IV:(n) + sec:[5].
  • Q88926733's catalog code is recorded as OGLE LMC175.5 17613[6].
  • Q88926733's catalog code is recorded as OGLE LMC553.25.036569[7].
  • Q88926733's catalog code is recorded as VFTS 314[8].
  • Q88926733's catalog code is recorded as IRSF J05382043-6903103[9].
  • Q88926733's catalog code is recorded as 2MASS J05382039-6903102[10].
  • Q88926733's catalog code is recorded as OGLE LMC-ECL-21259[11].
  • Q88926733's catalog code is recorded as Gaia DR2 4657686496901175424[12].
  • Q88926733's type of variable star is recorded as eclipsing binary star[13].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.06'}[14].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.09'}[15].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.08'}[16].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.07'}[17].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.07'}[18].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.972'}[19].
  • Q88926733's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.0830'}[20].
  • Q88926733's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0071'}[21].
  • Q88926733's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+179.2'}[22].
  • Q88926733's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+359.6'}[23].
  • Q88926733's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+122.6'}[24].
  • Q88926733's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+119.9'}[25].
  • Q88926733's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+364.6'}[26].

Body

Definition and Type

Q88926733's instance of is recorded as spectroscopic binary[2].

References

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

Direct Wikidata claims

  1. [2] . SIMBAD. wikidata.org.
  2. [3] . wikidata.org.
  3. [4] . The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. wikidata.org.
  4. [5] . The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. wikidata.org.
  5. [6] . SIMBAD. wikidata.org.
  6. [7] . SIMBAD. wikidata.org.
  7. [8] . SIMBAD. wikidata.org.
  8. [9] . SIMBAD. wikidata.org.
  9. [10] . SIMBAD. wikidata.org.
  10. [11] . SIMBAD. wikidata.org.
  11. [12] . SIMBAD. wikidata.org.
  12. [13] . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XII. Eclipsing binary stars in the Large Magellanic Cloud. wikidata.org.
  13. [14] . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  14. [15] . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  15. [16] . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  16. [17] . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  17. [18] . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  18. [19] . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XII. Eclipsing binary stars in the Large Magellanic Cloud. wikidata.org.
  19. [20] . Gaia Data Release 2. wikidata.org.
  20. [21] . Gaia Data Release 2. wikidata.org.
  21. [22] . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  22. [23] . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  23. [24] . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  24. [25] . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  25. [26] . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.

Class ancestry

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

📑 Cite this page

Use these citations when quoting this entity in research, articles, AI prompts, or wherever provenance matters. We aggregate Wikidata + Wikipedia + authoritative open-data sources; the stitched, scored, cross-referenced view is what 4ort.xyz contributes.

APA 4ort.xyz Knowledge Graph. (2026). Q88926733. Retrieved May 7, 2026, from https://4ort.xyz/entity/q88926733
MLA “Q88926733.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q88926733.
BibTeX @misc{4ortxyz_q88926733_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q88926733}}, year = {2026}, url = {https://4ort.xyz/entity/q88926733}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q88926733 — https://4ort.xyz/entity/q88926733 (retrieved 2026-05-07)

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