NGC 7752 and NGC 7753

(Redirected from Arp 86)

NGC 7752 and NGC 7753 are a pair of galaxies approximately 272 million light-years away in the constellation Pegasus.

NGC 7752 / 7753
NGC 7753 (big) and 7752 (small, bottom right)
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension23h 46m 58.5s / 23h 47m 04.8s[1]
Declination+29° 27′ 32″ / +29° 29′ 00″[1]
Heliocentric radial velocity5072 ± 5 / 5168 ± 6 km/s[1]
Distance272 Mly[2]
Apparent magnitude (V)15.0 / 12.8[1]
Characteristics
TypeI0 / SAB(rs)bc[1]
Apparent size (V)0.8 × 0.5 / 3.3 × 2.1[1]
Other designations
UGC 12779 / 12780,[1] PGC 72382 / 72387,[1] Arp 86[1]

NGC 7753 is the primary galaxy. It is a barred spiral galaxy with a small nucleus. NGC 7752 is the satellite galaxy of NGC 7753. It is a barred lenticular galaxy that is apparently attached to one of NGC 7753's spiral arms. They resemble the Whirlpool Galaxy (M51A) and its satellite NGC 5195 (M51B).

Supernovae

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The first supernova detected in NGC 7753 was SN 2006A in January 2006.[3] It was followed four months later by SN 2006ch, a Type Ia supernova.[3] In January 2013 another Type Ia supernova, SN 2013Q, was detected, and in August 2015 a Type II supernova, SN 2015ae, was discovered.[3]

See also

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References

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  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 7752 / 7753. Retrieved 2006-11-21.
  2. ^ Normandin, George. "NGC 7753 and NGC 7752 (aka Arp 86): Interacting Galaxies". Kopernik Observatory. Archived from the original on 3 March 2016. Retrieved 30 June 2015.
  3. ^ a b c "List of Supernovae". IAU Central Bureau for Astronomical Telegrams. IAU. Retrieved 19 February 2017.
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