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NGC 5394

NGC 5394
NGC 5394 (right) and NGC 5395 (left), as imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationCanes Venatici
Right ascension13h 58m 33s
Declination+37° 27’ 12”
Redshift0.011501
Heliocentric radial velocity3,448 km/s
Distance175 Mly (53.67 Mpc)
Apparent magnitude (B)13.7
Absolute magnitude (V)13.12
Surface brightness23.78 mag/arcsec^2
Characteristics
TypeSBb
Size96,900 ly (29.7 kpc estimated)
Apparent size (V)1.9' x 1.3'
Other designations
PGC 49739, UGC 8898, VV 48b, Arp 84, IRAS 13564+3741, MCG +06-31-033, CGCG 191-024

NGC 5394 is a barred spiral galaxy located in the constellation Canes Venatici. Its speed relative to the cosmic microwave background is 3,639 ± 14 km/s, which corresponds to a Hubble distance of 53.7 ± 3.8 Mpc (∼175 million ly).[1] NGC 5394 was discovered by German-British astronomer William Herschel in 1787.

The luminosity class of NGC 5394 is II and it has a broad HI line. It also contains regions of ionized hydrogen. It is also a Luminous Infrared Galaxy (LIRG).[1]

To date, one non-redshift-based measurement gives a distance of approximately 32,900 Mpc (∼107 million ly).[2] This value is far outside the Hubble distance values. Note that it is with the average value of independent measurements, when they exist, that the NASA/IPAC database calculates the diameter of a galaxy.

One supernova has been observed in NGC 5394: SN 2020aaxs (type Ib, mag. 17).[3]

Arp 84

NGC 5394 and NGC 5395 are a pair of gravitationally interacting galaxies that appear in Halton Arp's Atlas of Peculiar Galaxies under the designation Arp 84.[4] Arp noted that NGC 5495 is a spiral with a high surface luminosity companion at the end of one of its arms.[4]

NGC 5395 group

According to A.M. Garcia, NGC 5394 is part of a group of galaxies that has at least five members, the NGC 5395 group. The other galaxies are NGC 5341, NGC 5351, NGC 5395 and UGC 8806.[5]

See also

References

  1. ^ a b "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-07-24.
  2. ^ "NED Query Results for NGC 5393". ned.ipac.caltech.edu. Retrieved 2024-07-24.
  3. ^ Transient Name Server entry for SN 2020aaxs. Retrieved 23 July 2024.
  4. ^ a b Arp, Halton (1966-11-01). "Atlas of Peculiar Galaxies". The Astrophysical Journal Supplement Series. 14: 1. doi:10.1086/190147. ISSN 0067-0049.
  5. ^ Garcia, A. M. (1993-07-01). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. ISSN 0365-0138.

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