NGC 213 explained

NGC 213
Epoch:J2000
Ra:[1]
Constellation Name:Pisces
Z:0.018166
Dist Ly:NaNMpc
Type:SB(rs)a
Appmag V:14.23
Size V:1.7' × 1.4'

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]

One supernova has been observed in NGC 213: SN2020bqm (typeIa, mag. 18.4).[4]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 213 . 2016-09-02.
  2. Web site: New General Catalog Objects: NGC 200 - 249. Cseligman. September 14, 2016.
  3. NGC 213 . 5 September 2024 .
  4. Web site: Transient Name Server . SN2020bqm . . 4 September 2024.