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Q82947721

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Q82947721

Summary

Q82947721 is a T Tauri-type star[1].

Key Facts

  • Q82947721's instance of is recorded as T Tauri-type star[2].
  • Q82947721's constellation is recorded as Perseus[3].
  • Q82947721's spectral class is recorded as M5[4].
  • Q82947721's catalog code is recorded as Cl* IC 348 H 84[5].
  • Q82947721's catalog code is recorded as Cl* IC 348 HMW 146[6].
  • Q82947721's catalog code is recorded as Cl* IC 348 LRL 350[7].
  • Q82947721's catalog code is recorded as Cl* IC 348 LNB 118[8].
  • Q82947721's catalog code is recorded as 2MASS J03441918+3205599[9].
  • Q82947721's catalog code is recorded as IfAHA 86[10].
  • Q82947721's catalog code is recorded as SSTc2d J034419.2+320600[11].
  • Q82947721's catalog code is recorded as Cl* IC 348 CPS 33[12].
  • Q82947721's catalog code is recorded as [PSZ2003] J034419.2+320600[13].
  • Q82947721's catalog code is recorded as CXOU J034419.1+320600[14].
  • Q82947721's catalog code is recorded as Gaia DR2 216680756486417024[15].
  • Q82947721's apparent magnitude is recorded as {'unit': '1', 'amount': '+21.14'}[16].
  • Q82947721's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.855'}[17].
  • Q82947721's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.386'}[18].
  • Q82947721's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.582'}[19].
  • Q82947721's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.21'}[20].
  • Q82947721's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.5735'}[21].
  • Q82947721's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.1209'}[22].
  • Q82947721's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+16.868431000'}[23].
  • Q82947721's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+16.868431'}[24].
  • Q82947721's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.956830'}[25].
  • Q82947721's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+23.21'}[26].

Body

Definition and Type

Q82947721's instance of is recorded as T Tauri-type 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] ↑ . Deep MIPS observations of the IC 348 nebula: constraints on the evolutionary state of anemic circumstellar disks and the primordial-to-debris disk transition. 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] ↑ . Do accretion discs regulate the rotation of young stars?. 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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  23. [24] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  24. [25] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  25. [26] ↑ . IN-SYNC I: homogeneous stellar parameters from high-resolution APOGEE spectra for thousands of pre-main sequence 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). Q82947721. Retrieved May 7, 2026, from https://4ort.xyz/entity/q82947721
MLA “Q82947721.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q82947721.
BibTeX @misc{4ortxyz_q82947721_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q82947721}}, year = {2026}, url = {https://4ort.xyz/entity/q82947721}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q82947721 — https://4ort.xyz/entity/q82947721 (retrieved 2026-05-07)

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