Q88627417

emission-line star in the constellation Mensa
Thing emission_line_star Q88627417
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Q88627417

Summary

Q88627417 is an emission-line star[1].

Key Facts

  • Q88627417's instance of is recorded as emission-line star[2].
  • Q88627417's constellation is recorded as Mensa[3].
  • Q88627417's spectral class is recorded as B0III[e][4].
  • Q88627417's catalog code is recorded as OGLE LMC137.1 9867[5].
  • Q88627417's catalog code is recorded as OGLE LMC530.11.007532[6].
  • Q88627417's catalog code is recorded as GSC 09165-00926[7].
  • Q88627417's catalog code is recorded as 2MASS J04532543-7035395[8].
  • Q88627417's catalog code is recorded as SK -70 10[9].
  • Q88627417's catalog code is recorded as [M2002] LMC 16948[10].
  • Q88627417's catalog code is recorded as OGLE LMC-ECL-2253[11].
  • Q88627417's catalog code is recorded as [GC2009] J045325.51-703541.2[12].
  • Q88627417's catalog code is recorded as [WSI2008] 80[13].
  • Q88627417's catalog code is recorded as SSTISAGE1C J045325.57-703541.2[14].
  • Q88627417's catalog code is recorded as [RP2006] 1671[15].
  • Q88627417's catalog code is recorded as UCAC4 098-005101[16].
  • Q88627417's catalog code is recorded as [H2013] LMCe 68[17].
  • Q88627417's catalog code is recorded as Gaia DR2 4654738633163743232[18].
  • Q88627417's type of variable star is recorded as eclipsing binary star[19].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.896'}[20].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.775'}[21].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.824'}[22].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.770'}[23].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2'}[24].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.500'}[25].
  • Q88627417's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.915'}[26].

Body

Definition and Type

Q88627417's instance of is recorded as emission-line star[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] . Emission-line stars discovered in the UKST h{alpha} survey of the large Magellanic cloud -- I. Hot stars. 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] . SIMBAD. wikidata.org.
  15. [16] . SIMBAD. wikidata.org.
  16. [17] . SIMBAD. wikidata.org.
  17. [18] . SIMBAD. wikidata.org.
  18. [19] . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XII. Eclipsing binary stars in the Large Magellanic Cloud. wikidata.org.
  19. [20] . Emission-line stars discovered in the UKST h{alpha} survey of the large Magellanic cloud -- I. Hot stars. wikidata.org.
  20. [21] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  21. [22] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  22. [23] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  23. [24] . A deep objective-prism survey for Large Magellanic Cloud members. wikidata.org.
  24. [25] . The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. XII. Eclipsing binary stars in the Large Magellanic Cloud. wikidata.org.
  25. [26] . Emission-line stars discovered in the UKST h{alpha} survey of the large Magellanic cloud -- I. Hot stars. 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). Q88627417. Retrieved May 7, 2026, from https://4ort.xyz/entity/q88627417
MLA “Q88627417.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q88627417.
BibTeX @misc{4ortxyz_q88627417_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q88627417}}, year = {2026}, url = {https://4ort.xyz/entity/q88627417}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q88627417 — https://4ort.xyz/entity/q88627417 (retrieved 2026-05-07)

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