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NGC 213

From Wikipedia, the free encyclopedia
NGC 213
SDSS image of NGC 213
Observation data (J2000 epoch)
ConstellationPisces
Right ascension00h 41m 09.9940s[1]
Declination+16° 28 09.508[1]
Redshift0.018166[1]
Distance245.7 ± 17.2 Mly (75.32 ± 5.28 Mpc)[1]
Apparent magnitude (V)14.23[1]
Characteristics
TypeSB(rs)a[1]
Apparent size (V)1.7' × 1.4'[1]
Other designations
IRAS F00384+1611, 2MASX J00411000+1628101, UGC 436, MCG +03-02-023, PGC 2469, CGCG 457-026[1]

NGC 213 is a barred spiral galaxy located in the constellation Pisces. It was discovered on October 14, 1784, by William Herschel.[2]

According to the SIMBAD database, NGC 213 is an Active Galaxy Nucleus Candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[3]

Supernova

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One supernova has been observed in NGC 213:

  • SN 2020bqm (Type Ia, mag. 18.389) was discovered by ATLAS on 2 February 2020.[4]

See also

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References

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  1. 1 2 3 4 5 6 7 8 "Results for object NGC 0213". NASA/IPAC Extragalactic Database. Retrieved 2016-09-02.
  2. "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 14, 2016.
  3. "NGC 213". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 5 September 2024.
  4. "SN 2020bqm". Transient Name Server. IAU. Retrieved 4 September 2024.