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Q86119128

spectroscopic binary in the constellation Dorado
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Q86119128

Summary

Q86119128 is a spectroscopic binary[1].

Key Facts

  • Q86119128's instance of is recorded as spectroscopic binary[2].
  • Q86119128's constellation is recorded as Dorado[3].
  • Q86119128's spectral class is recorded as O9/B0[4].
  • Q86119128's spectral class is recorded as O9.7 II or B0 IV ?[5].
  • Q86119128's catalog code is recorded as [M2002] LMC 168939[6].
  • Q86119128's catalog code is recorded as [ST92] 1-39[7].
  • Q86119128's catalog code is recorded as 2MASS J05374092-6908442[8].
  • Q86119128's catalog code is recorded as SSTISAGEMC J053740.92-690844.4[9].
  • Q86119128's catalog code is recorded as IRSF J05374090-6908443[10].
  • Q86119128's catalog code is recorded as VFTS 113[11].
  • Q86119128's catalog code is recorded as Gaia DR2 4657690310833117312[12].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.052'}[13].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.829'}[14].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.633'}[15].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.491'}[16].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.27'}[17].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.20'}[18].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.12'}[19].
  • Q86119128's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.7412'}[20].
  • Q86119128's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0315'}[21].
  • Q86119128's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+281.8'}[22].
  • Q86119128's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+281.0'}[23].
  • Q86119128's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+275.7'}[24].
  • Q86119128's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+272.8'}[25].
  • Q86119128's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+269.3'}[26].

Body

Definition and Type

Q86119128'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] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  13. [14] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  14. [15] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. wikidata.org.
  15. [16] ↑ . Spitzer SAGE infrared photometry of massive stars in the Large Magellanic Cloud. 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 VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. 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). Q86119128. Retrieved May 7, 2026, from https://4ort.xyz/entity/q86119128
MLA “Q86119128.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q86119128.
BibTeX @misc{4ortxyz_q86119128_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q86119128}}, year = {2026}, url = {https://4ort.xyz/entity/q86119128}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q86119128 — https://4ort.xyz/entity/q86119128 (retrieved 2026-05-07)

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