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Galaxy in the constellation Pegasus

NGC 7549

NGC 7549
All data from the card 11
Constellation
Pegasus
Right ascension
23h 15m 17.2735s
Declination
+19° 02′ 30.087″
Redshift
0.015798±0.00001
Heliocentric radial velocity
4,736±3 km/s
Distance
187.41 ± 14.74 Mly (57.460 ± 4.518 Mpc)
Group or cluster
Arp 99, HCG 93
Apparent magnitude (V)
13.74
Type
SB(s)cd pec
Size
~160,900 ly (49.34 kpc) (estimated)
Apparent size (V)
2.8′ × 0.7′

NGC 7549 is a peculiar barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 4,373±26 km/s, which corresponds to a Hubble distance of 210.4 ± 14.8 Mly (64.50 ± 4.53 Mpc). However, five non-redshift measurements give a closer mean distance of 187.41 ± 14.74 Mly (57.460 ± 4.518 Mpc). It was discovered by Irish engineer Bindon Stoney on 2 November 1850.

NGC 7549 has an active galactic nucleus, 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.

Hickson Compact Group 93

HCG 93 imaged by Legacy Surveys
HCG 93 imaged by Legacy Surveys
HCG 93 imaged by SDSS
HCG 93 imaged by SDSS
2 images

NGC 7549 is a member of the Hickson Compact Group HCG 93. This five member group of galaxies also contains NGC 7547, NGC 7550, NGC 7553, and NGC 7558.

Arp 99

NGC 7549 along with NGC 7547 and NGC 7550 are listed together as Arp 99 in Halton Arp's Atlas of Peculiar Galaxies as Arp 99, as an example of spirals with companions attached to spiral arms.

Supernovae

Two supernovae have been observed in NGC 7549:

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Text from Wikipedia, CC BY-SA 4.0 · Source article