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Q89067682

young stellar object candidate in the constellation Perseus
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Q89067682

Summary

Q89067682 is a young stellar object candidate[1].

Key Facts

  • Q89067682's instance of is recorded as young stellar object candidate[2].
  • Q89067682's constellation is recorded as Perseus[3].
  • Q89067682's catalog code is recorded as SSTc2d J034157.4+314837[4].
  • Q89067682's catalog code is recorded as [EDJ2009] 314[5].
  • Q89067682's catalog code is recorded as 2MASS J03415745+3148365[6].
  • Q89067682's catalog code is recorded as SSTc2d J034157.4+314836[7].
  • Q89067682's catalog code is recorded as [HL2013] 055.48934+31.81021[8].
  • Q89067682's catalog code is recorded as Gaia DR2 216587371012705792[9].
  • Q89067682's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.095'}[10].
  • Q89067682's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.599'}[11].
  • Q89067682's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.655'}[12].
  • Q89067682's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.4518'}[13].
  • Q89067682's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.7438'}[14].
  • Q89067682's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.686523000'}[15].
  • Q89067682's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.050818'}[16].
  • Q89067682's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+16.302032'}[17].
  • Q89067682's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.686523'}[18].
  • Q89067682's SIMBAD ID is recorded as ZTF J034157.46+314836.5[19].
  • Q89067682's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+40.54'}[20].
  • Q89067682's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+55.48942663422210'}[21].
  • Q89067682's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+31.81016667480180'}[22].
  • Q89067682's epoch is recorded as J2000.0[23].
  • Q89067682's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4063'}[24].
  • Q89067682's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+6900'}[25].
  • Q89067682's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.957'}[26].

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] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  10. [11] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  11. [12] ↑ . VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003). wikidata.org.
  12. [13] ↑ . Gaia Data Release 2. wikidata.org.
  13. [14] ↑ . Gaia Data Release 2. wikidata.org.
  14. [15] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  15. [16] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  16. [17] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  17. [18] ↑ . IN-SYNC. III. The dynamical state of IC 348 - a super-virial velocity dispersion and a puzzling sign of convergence. wikidata.org.
  18. [19] ↑ . wikidata.org.
  19. [20] ↑ . IN-SYNC I: homogeneous stellar parameters from high-resolution APOGEE spectra for thousands of pre-main sequence stars. wikidata.org.
  20. [21] ↑ . Gaia Data Release 2. wikidata.org.
  21. [22] ↑ . Gaia Data Release 2. wikidata.org.
  22. [23] ↑ . Gaia Data Release 2. wikidata.org.
  23. [24] ↑ . IN-SYNC I: homogeneous stellar parameters from high-resolution APOGEE spectra for thousands of pre-main sequence stars. wikidata.org.
  24. [25] ↑ . IN-SYNC I: homogeneous stellar parameters from high-resolution APOGEE spectra for thousands of pre-main sequence stars. 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). Q89067682. Retrieved May 7, 2026, from https://4ort.xyz/entity/q89067682
MLA “Q89067682.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q89067682.
BibTeX @misc{4ortxyz_q89067682_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q89067682}}, year = {2026}, url = {https://4ort.xyz/entity/q89067682}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q89067682 — https://4ort.xyz/entity/q89067682 (retrieved 2026-05-07)

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