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Q94190764

spectroscopic binary in the constellation Dorado
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Q94190764

Summary

Q94190764 is a spectroscopic binary[1].

Key Facts

  • Q94190764's instance of is recorded as spectroscopic binary[2].
  • Q94190764's constellation is recorded as Dorado[3].
  • Q94190764's spectral class is recorded as O5.5V((n))((f))z[4].
  • Q94190764's spectral class is recorded as O5.5[5].
  • Q94190764's spectral class is recorded as O5.5 V((n))((f))z[6].
  • Q94190764's catalog code is recorded as Cl* NGC 2070 MEL 59a[7].
  • Q94190764's catalog code is recorded as [P93] 341[8].
  • Q94190764's catalog code is recorded as VFTS 398[9].
  • Q94190764's catalog code is recorded as IRSF J05383338-6904384[10].
  • Q94190764's catalog code is recorded as Gaia DR2 4657686325102027648[11].
  • Q94190764's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.40'}[12].
  • Q94190764's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.37'}[13].
  • Q94190764's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.34'}[14].
  • Q94190764's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.40'}[15].
  • Q94190764's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.41'}[16].
  • Q94190764's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.3345'}[17].
  • Q94190764's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.9642'}[18].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+270.7'}[19].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+273.3'}[20].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+271.7'}[21].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+268.4'}[22].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+269.2'}[23].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+267.0'}[24].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+264.1'}[25].
  • Q94190764's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+265.8'}[26].

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. XIII: On the nature of O Vz stars in 30 Doradus. wikidata.org.
  5. [6] ↑ . The VLT-FLAMES Tarantula Survey. XIV. The O-type stellar content of 30 Doradus. 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] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. wikidata.org.
  12. [13] ↑ . The VLT-FLAMES Tarantula Survey. I. Introduction and observational overview. 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] ↑ . Gaia Data Release 2. wikidata.org.
  17. [18] ↑ . Gaia Data Release 2. wikidata.org.
  18. [19] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  19. [20] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. wikidata.org.
  20. [21] ↑ . The VLT-FLAMES Tarantula Survey. VIII. Multiplicity properties of the O-type star population. 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). Q94190764. Retrieved May 7, 2026, from https://4ort.xyz/entity/q94190764
MLA “Q94190764.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q94190764.
BibTeX @misc{4ortxyz_q94190764_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q94190764}}, year = {2026}, url = {https://4ort.xyz/entity/q94190764}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q94190764 — https://4ort.xyz/entity/q94190764 (retrieved 2026-05-07)

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