Supriya Ghosh (Editor)

NGC 4088

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Right ascension
  
12 05 34.2

Redshift
  
0.002524

Type
  
SAB(rs)bc

Constellation
  
Declination
  
+50° 32′ 21″

Helio radial velocity
  
757 ± 1 km/s

Magnitude
  
11.2

Apparent magnitude (V)
  
11.2


Distance
  
51.5 ± 4.5 Mly(15.8 ± 1.4 Mpc)

Similar
  
NGC 4041, NGC 4102, NGC 4194, NGC 3953, NGC 4036

NGC 4088 is an intermediate spiral galaxy in the constellation Ursa Major. The galaxy forms a physical pair with NGC 4085, which is located 11′ away.

NGC 4088 is a grand design spiral galaxy. This means that the spiral arms in the galaxy's disk are sharply defined. In visible light, one of the spiral arms appears to have a disconnected segment. Halton Arp included this galaxy in the Atlas of Peculiar Galaxies as one of several examples where this phenomenon occurs.

NGC 4088 and NGC 4085 are members of the M109 Group, a group of galaxies located in the constellation Ursa Major. This large group contains between 41 and 58 galaxies, including the spiral galaxy M109.

Supernova 2009dd

On April 13, 2009, SN 2009dd was discovered in NGC 4088. At apparent magnitude 13.8, it became the third-brightest supernova of 2009. In 1991 there was SN1991G.

References

NGC 4088 Wikipedia


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