KPG 239

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KPG 239
NGC 3286 and NGC 3288
NGC3284 - SDSS DR14.png

NGC3288 - SDSS DR14.jpg
KPG 239A (NGC 3286) above and KPG 239B (NGC 3288) below ( SDSS images)
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Ursa Major
Right ascension 10 h 36.4 m
declination 2583500+ 58 ° 35 ′ 0 ″
Apparent brightness
(V-band)
A. approx. 13.6 mag
B. approx. 13.8 mag
Apparent brightness
(B-band)
A. about 14.3 mag
B. approx 14.5 mag
Physical data
Heliocentric radial velocity A. (8094 ± 47) km / s
B. 8151 ± 56 km / s
distance approx. 110 M pc
Catalog entries
KPG 239A / NGC  3286 : CGCG  290-56 • MCG  + 10-15-112 • PGC  31433

KPG 239B / NGC 3288 : UGC  5752 • CGCG 290-57 • MCG + 10-15-114 • PGC 31446 • IRAS F10332 + 5849

KPG 239 (also CPG 239 ) is a pair of galaxies in the constellation Ursa Major around 110 million parsecs away. The pair consists of two galaxies separated by about 4  arc minutes with similar apparent brightness. The pair does not form an isolated system, but there are several other galaxies in the same field, among which these two stand out most clearly.

The more northerly component, KPG 239A or NGC 3286 , is classified as an elliptical to lenticular galaxy (E3 / S0 pec), while the more southerly, KPG 239B or NGC 3288 , is classified as a spiral galaxy (Sb pec). At KPG 239B there is an arcuate spiral arm tapering to the south. KPG 239A is a powerful X-ray source.

literature

  • M. Henriksen, S. Cousineau: An X-Ray Survey of Galaxies in Pairs. In: The Astrophysical Journal. Volume 511, No. 2, 1999, pp. 595-611.
  • A. Franco-Balderas, HM Hernández-Toledo, D. Dultzin-Hacyan: BVRI surface photometry of mixed morphology pairs of galaxies. II. The second data set. In: Astronomy and Astrophysics. Volume 417, 2004, pp. 411-419.
  • HM Hernández-Toledo, V. Avila-Reese, JR Salazar-Contreras, CJ Conselice: The Effects of Interactions on the Structure and Morphology of Elliptical / Lenticular Galaxies in Pairs. In: The Astronomical Journal. Volume 132, No. 1, 2006, pp. 71-84.