Q80406928

carbon star in the constellation Pyxis
Thing carbon_star Q80406928
Press Enter · cited answer in seconds

Q80406928

Summary

Q80406928 is a carbon star[1].

Key Facts

  • Q80406928's instance of is recorded as carbon star[2].
  • Q80406928's constellation is recorded as Pyxis[3].
  • Q80406928's spectral class is recorded as C-rich[4].
  • Q80406928's catalog code is recorded as AN 406.1933[5].
  • Q80406928's catalog code is recorded as C* 1293[6].
  • Q80406928's catalog code is recorded as CD-33 5429[7].
  • Q80406928's catalog code is recorded as CGCS 2334[8].
  • Q80406928's catalog code is recorded as CSV 1368[9].
  • Q80406928's catalog code is recorded as HIC 43123[10].
  • Q80406928's catalog code is recorded as HIP 43123[11].
  • Q80406928's catalog code is recorded as Hen 3-205[12].
  • Q80406928's catalog code is recorded as IRAS 08450-3407[13].
  • Q80406928's catalog code is recorded as ASAS J084700-3419.0[14].
  • Q80406928's catalog code is recorded as SV* HV 8161[15].
  • Q80406928's catalog code is recorded as SV* P 574[16].
  • Q80406928's catalog code is recorded as YC Red 13[17].
  • Q80406928's catalog code is recorded as [ELL90] 81[18].
  • Q80406928's catalog code is recorded as 2MASS J08470016-3418589[19].
  • Q80406928's catalog code is recorded as TYC 7145-295-1[20].
  • Q80406928's catalog code is recorded as Gaia DR1 5627021235006515456[21].
  • Q80406928's catalog code is recorded as Gaia DR2 5627021239308538880[22].
  • Q80406928's catalog code is recorded as UW Pyx[23].
  • Q80406928's type of variable star is recorded as long-period variable star[24].
  • Q80406928's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.87'}[25].
  • Q80406928's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.46'}[26].

Body

Definition and Type

Q80406928's instance of is recorded as carbon 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] . Classification and Identification of IRAS Sources with Low-Resolution Spectra. 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] . SIMBAD. wikidata.org.
  19. [20] . SIMBAD. wikidata.org.
  20. [21] . SIMBAD. wikidata.org.
  21. [22] . SIMBAD. wikidata.org.
  22. [23] . wikidata.org.
  23. [24] . Determination of pulsation periods and other parameters of 2875 stars classified as Mira in the All Sky Automated Survey (ASAS). wikidata.org.
  24. [25] . Near-infrared photometry of carbon stars. wikidata.org.
  25. [26] . Near-infrared photometry of carbon 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). Q80406928. Retrieved May 7, 2026, from https://4ort.xyz/entity/q80406928
MLA “Q80406928.” 4ort.xyz Knowledge Graph, 4ort.xyz, 7 May. 2026, https://4ort.xyz/entity/q80406928.
BibTeX @misc{4ortxyz_q80406928_2026, author = {{4ort.xyz Knowledge Graph}}, title = {{Q80406928}}, year = {2026}, url = {https://4ort.xyz/entity/q80406928}, note = {Accessed: 2026-05-07}}
LLM prompt According to 4ort.xyz Knowledge Graph (aggregator of Wikidata, Wikipedia, and authoritative open-data sources): Q80406928 — https://4ort.xyz/entity/q80406928 (retrieved 2026-05-07)

Canonical URL: https://4ort.xyz/entity/q80406928 · Last refreshed: