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NGC 5875

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Galaxy in the constellation Boötes

NGC 5875
The spiral galaxy NGC 5875
Observation data (J2000 epoch)
ConstellationBoötes
Right ascension15 09 13.1946
Declination+52° 31′ 42.472″
Redshift0.011695
Heliocentric radial velocity3506 ± 2 km/s
Distance172.4 ± 12.1 Mly (52.87 ± 3.70 Mpc)
Apparent magnitude (V)12.4
Characteristics
TypeSAb?
Size~116,800 ly (35.80 kpc) (estimated)
Apparent size (V)2.3′ × 1.2′
Other designations
IRAS 15077+5243, 2MASX J15091320+5231418, UGC 9745, MCG +09-25-027, PGC 54095, CGCG 274-027

NGC 5875 is a spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3585 ± 6 km/s, which corresponds to a Hubble distance of 52.87 ± 3.70 Mpc (∼173 million light-years). It was discovered by German-British astronomer William Herschel on 1 May 1788.

The SIMBAD database lists NGC 5875 as a Seyfert II Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.

Two supernovae have been observed in NGC 5875:

See also

References

  1. ^ "Results for object NGC 5875". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 7 August 2024.
  2. Seligman, Courtney. "New General Catalogue Objects: NGC 5875". Celestial Atlas. Retrieved 14 December 2024.
  3. "NGC 5875". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 December 2024.
  4. "SN 2022oqm". Transient Name Server. IAU. Retrieved 16 December 2024.
  5. Yadavalli, S. Karthik; et al. (2024). "SN 2022oqm: A Bright and Multipeaked Calcium-rich Transient". The Astrophysical Journal. 972 (2): 194. arXiv:2308.12991. Bibcode:2024ApJ...972..194Y. doi:10.3847/1538-4357/ad5a7c.
  6. "SN 2023ldh". Transient Name Server. IAU. Retrieved 16 December 2024.

External links

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