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Q94190560

spectroscopic binary in the constellation Dorado
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Q94190560

Summary

Q94190560 is a spectroscopic binary[1].

Key Facts

  • Q94190560's instance of is recorded as spectroscopic binary[2].
  • Q94190560's constellation is recorded as Dorado[3].
  • Q94190560's spectral class is recorded as O9.5IV[4].
  • Q94190560's spectral class is recorded as O9.5 IV[5].
  • Q94190560's catalog code is recorded as [P93] 1468[6].
  • Q94190560's catalog code is recorded as IRSF J05384904-6906196[7].
  • Q94190560's catalog code is recorded as Cl* NGC 2070 SMB 174[8].
  • Q94190560's catalog code is recorded as VFTS 635[9].
  • Q94190560's catalog code is recorded as Gaia DR2 4657685534828291072[10].
  • Q94190560's catalog code is recorded as [CCE2018] 1334[11].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.52'}[12].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.59'}[13].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.47'}[14].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.44'}[15].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.45'}[16].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.5421'}[17].
  • Q94190560's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.54'}[18].
  • Q94190560's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0033'}[19].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+260.7'}[20].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+260.1'}[21].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+263.7'}[22].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+258.3'}[23].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+258.6'}[24].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+263.3'}[25].
  • Q94190560's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+265.2'}[26].

Body

Definition and Type

Q94190560'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] ↑ . 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] ↑ . Mapping the core of the Tarantula Nebula with VLT-MUSE. I. Spectral and nebular content around R136. wikidata.org.
  18. [19] ↑ . Gaia Data Release 2. 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). Q94190560. Retrieved May 7, 2026, from https://4ort.xyz/entity/q94190560
MLA “Q94190560.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q94190560.
BibTeX @misc{4ortxyz_q94190560_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q94190560}}, year = {2026}, url = {https://4ort.xyz/entity/q94190560}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q94190560 — https://4ort.xyz/entity/q94190560 (retrieved 2026-05-07)

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