Q90906414

spectroscopic binary in the constellation Gemini
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Q90906414

Summary

Q90906414 is a spectroscopic binary[1].

Key Facts

  • Q90906414's instance of is recorded as spectroscopic binary[2].
  • Q90906414's constellation is recorded as Gemini[3].
  • Q90906414's catalog code is recorded as 2MASS J06085043+2422305[4].
  • Q90906414's catalog code is recorded as Cl* NGC 2168 BSB 5042[5].
  • Q90906414's catalog code is recorded as Cl* NGC 2168 M 150[6].
  • Q90906414's catalog code is recorded as Cl* NGC 2168 CD 334[7].
  • Q90906414's catalog code is recorded as Cl* NGC 2168 SB 518[8].
  • Q90906414's catalog code is recorded as Cl* NGC 2168 CUD 180[9].
  • Q90906414's catalog code is recorded as NGC 2168 121[10].
  • Q90906414's catalog code is recorded as [GMB2010] WOCS 16009[11].
  • Q90906414's catalog code is recorded as [SLB2011b] 092.21008+24.37531[12].
  • Q90906414's catalog code is recorded as SDSS J060850.43+242230.4[13].
  • Q90906414's catalog code is recorded as Gaia DR2 3426270990284957056[14].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.992'}[15].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.139'}[16].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.556'}[17].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.266'}[18].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.189'}[19].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.68'}[20].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.710'}[21].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.612'}[22].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.191'}[23].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.148'}[24].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.157'}[25].
  • Q90906414's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.8041'}[26].

Body

Definition and Type

Q90906414'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] . SIMBAD. wikidata.org.
  4. [5] . SIMBAD. 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] . SIMBAD. wikidata.org.
  13. [14] . SIMBAD. wikidata.org.
  14. [15] . From the Top to the Bottom of the Main Sequence: A Complete Mass Function of the Young Open Cluster M35. wikidata.org.
  15. [16] . From the Top to the Bottom of the Main Sequence: A Complete Mass Function of the Young Open Cluster M35. wikidata.org.
  16. [17] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  17. [18] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  18. [19] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  19. [20] . WIYN open cluster study. XXXVIII. Stellar radial velocities in the young open cluster M35 (NGC 2168). wikidata.org.
  20. [21] . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  21. [22] . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  22. [23] . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  23. [24] . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  24. [25] . The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. wikidata.org.
  25. [26] . Gaia Data Release 2. 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). Q90906414. Retrieved May 7, 2026, from https://4ort.xyz/entity/q90906414
MLA “Q90906414.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q90906414.
BibTeX @misc{4ortxyz_q90906414_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q90906414}}, year = {2026}, url = {https://4ort.xyz/entity/q90906414}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q90906414 — https://4ort.xyz/entity/q90906414 (retrieved 2026-05-07)

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