WR 9

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WR 9

Summary

WR 9 is a star[1]. It ranks in the top 6% of star entities by monthly Wikipedia readership (5 views/month).[2]

Key Facts

  • WR 9's instance of is recorded as star[3].
  • WR 9's instance of is recorded as eclipsing binary star[4].
  • WR 9's instance of is recorded as spectroscopic binary[5].
  • WR 9's instance of is recorded as Wolf–Rayet star[6].
  • WR 9's instance of is recorded as infrared source[7].
  • WR 9's constellation is recorded as Puppis[8].
  • WR 9's spectral class is recorded as WC4+O7[9].
  • WR 9's catalog code is recorded as HD 63099[10].
  • WR 9's catalog code is recorded as GSC 07114-00644[11].
  • WR 9's catalog code is recorded as 2MASS J07455041-3419483[12].
  • WR 9's catalog code is recorded as HIP 37876[13].
  • WR 9's catalog code is recorded as IC 2206[14].
  • WR 9's catalog code is recorded as ALS 753[15].
  • WR 9's catalog code is recorded as CD-34 3879[16].
  • WR 9's catalog code is recorded as CPD-34 1643[17].
  • WR 9's catalog code is recorded as HIC 37876[18].
  • WR 9's catalog code is recorded as TYC 7114-644-1[19].
  • WR 9's catalog code is recorded as UBV M 13621[20].
  • WR 9's catalog code is recorded as V443 Pup[21].
  • WR 9's catalog code is recorded as UCAC4 279-023617[22].
  • WR 9's catalog code is recorded as SBC9 476[23].
  • WR 9's catalog code is recorded as Gaia DR1 5588584473161108992[24].
  • WR 9's catalog code is recorded as WEB 7477[25].
  • WR 9's catalog code is recorded as Gaia DR2 5588584477463342592[26].
  • WR 9's apparent magnitude is recorded as {'amount': '+11.47'}[27].

Body

Designation and Status

Recorded instance of include star[3], eclipsing binary star[4], spectroscopic binary[5], Wolf–Rayet star[6], and infrared source[7].

History and Context

Catalog codes include HD 63099[10], GSC 07114-00644[11], 2MASS J07455041-3419483[12], HIP 37876[13], IC 2206[14], and ALS 753[15].

Why It Matters

WR 9 ranks in the top 6% of star entities by monthly Wikipedia readership (5 views/month).[2]

References

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

Direct Wikidata claims

  1. [3] . SIMBAD. wikidata.org.
  2. [4] . SIMBAD. wikidata.org.
  3. [5] . SIMBAD. wikidata.org.
  4. [6] . SIMBAD. wikidata.org.
  5. [7] . SIMBAD. wikidata.org.
  6. [8] . VizieR. wikidata.org.
  7. [9] . Magellanic Cloud WC/WO Wolf-Rayet stars - I. Binary frequency and Roche lobe overflow formation. wikidata.org.
  8. [10] . SIMBAD. wikidata.org.
  9. [11] . SIMBAD. wikidata.org.
  10. [12] . SIMBAD. wikidata.org.
  11. [13] . SIMBAD. wikidata.org.
  12. [14] . SIMBAD. wikidata.org.
  13. [15] . SIMBAD. wikidata.org.
  14. [16] . SIMBAD. wikidata.org.
  15. [17] . SIMBAD. wikidata.org.
  16. [18] . SIMBAD. wikidata.org.
  17. [19] . SIMBAD. wikidata.org.
  18. [20] . SIMBAD. wikidata.org.
  19. [21] . SIMBAD. wikidata.org.
  20. [22] . SIMBAD. wikidata.org.
  21. [23] . SIMBAD. wikidata.org.
  22. [24] . SIMBAD. wikidata.org.
  23. [25] . SIMBAD. wikidata.org.
  24. [26] . SIMBAD. wikidata.org.
  25. [27] . Catalogue of Stellar Photometry in Johnson's 11-color system. wikidata.org.

Class ancestry

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

Aggregate / graph-position facts

  1. [2] . Wikimedia Foundation. dumps.wikimedia.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). WR 9. Retrieved May 3, 2026, from https://4ort.xyz/entity/wr-9
MLA “WR 9.” 4ort.xyz Knowledge Graph, 4ort.xyz, 3 May. 2026, https://4ort.xyz/entity/wr-9.
BibTeX @misc{4ortxyz_wr-9_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{WR 9}}, year = {2026}, url = {https://4ort.xyz/entity/wr-9}, note = {Accessed: 2026-05-03}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): WR 9 — https://4ort.xyz/entity/wr-9 (retrieved 2026-05-03)

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