Q85056640

Thing t_tauri_type_star Q85056640
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Q85056640

Summary

Q85056640 is a T Tauri-type star[1].

Key Facts

  • Q85056640's instance of is recorded as T Tauri-type star[2].
  • Q85056640's instance of is recorded as emission-line star[3].
  • Q85056640's instance of is recorded as galaxy[4].
  • Q85056640's instance of is recorded as near-infrared source[5].
  • Q85056640's instance of is recorded as variable star[6].
  • Q85056640's instance of is recorded as astrophysical X-ray source[7].
  • Q85056640's constellation is recorded as Monoceros[8].
  • Q85056640's spectral class is recorded as M2.5[9].
  • Q85056640 is part of Q226134[10].
  • Q85056640's catalog code is recorded as 2MASS J06411792+0929011[11].
  • Q85056640's catalog code is recorded as NSV 17116[12].
  • Q85056640's catalog code is recorded as IPHAS J064117.93+092901.1[13].
  • Q85056640's catalog code is recorded as Gaia DR2 3326692276606374144[14].
  • Q85056640's catalog code is recorded as V821 Mon[15].
  • Q85056640's catalog code is recorded as TIC 220338508[16].
  • Q85056640's catalog code is recorded as Gaia DR3 3326692276606374144[17].
  • Q85056640's type of variable star is recorded as Orion variable[18].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.43'}[19].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.05'}[20].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.55'}[21].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+23.007'}[22].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.637'}[23].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.508'}[24].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.167'}[25].
  • Q85056640's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.33'}[26].

Body

Definition and Type

Recorded instance of include T Tauri-type star[2], emission-line star[3], galaxy[4], near-infrared source[5], variable star[6], and astrophysical X-ray source[7].

Use and Application

Q85056640 is part of Q226134[10].

References

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

Direct Wikidata claims

  1. [2] . SIMBAD. wikidata.org.
  2. [3] . SIMBAD. wikidata.org.
  3. [4] . SIMBAD. wikidata.org.
  4. [5] . SIMBAD. wikidata.org.
  5. [6] . SIMBAD. wikidata.org.
  6. [7] . SIMBAD. wikidata.org.
  7. [8] . wikidata.org.
  8. [9] . ACIS-I observations of NGC 2264. Membership and X-ray properties of PMS stars. 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] . Q56001295. wikidata.org.
  18. [19] . ACIS-I observations of NGC 2264. Membership and X-ray properties of PMS stars. wikidata.org.
  19. [20] . ACIS-I observations of NGC 2264. Membership and X-ray properties of PMS stars. wikidata.org.
  20. [21] . Accretion dynamics and disk evolution in NGC 2264: a study based on CoRoT photometric observations. wikidata.org.
  21. [22] . Mapping accretion and its variability in the young open cluster NGC 2264: a study based onu-band photometry. wikidata.org.
  22. [23] . Mapping accretion and its variability in the young open cluster NGC 2264: a study based onu-band photometry. wikidata.org.
  23. [24] . Mapping accretion and its variability in the young open cluster NGC 2264: a study based onu-band photometry. wikidata.org.
  24. [25] . Mapping accretion and its variability in the young open cluster NGC 2264: a study based onu-band photometry. wikidata.org.
  25. [26] . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). 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). Q85056640. Retrieved May 7, 2026, from https://4ort.xyz/entity/q85056640
MLA “Q85056640.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q85056640.
BibTeX @misc{4ortxyz_q85056640_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q85056640}}, year = {2026}, url = {https://4ort.xyz/entity/q85056640}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q85056640 — https://4ort.xyz/entity/q85056640 (retrieved 2026-05-07)

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