NGC 7742
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| NGC 7742 | |
 A Hubble Space Telescope (HST) image of NGC 7742. Credit: HST/NASA/ESA. |
|
| Observation data (J2000 epoch) | |
|---|---|
| Constellation | Pegasus |
| Right ascension | 23h 44m 15.7s[1] |
| Declination | +10° 46′ 02″[1] |
| Redshift | 1663 km/s[1] |
| Distance | 72 Mly (22 Mpc)[2] |
| Type | SA(r)b[1] |
| Apparent dimensions (V) | 1′.7×1′.7[1] |
| Apparent magnitude (V) | 12.4[1] |
| Other designations | |
| UGC 12760,[1] PGC 72260[1] | |
| See also: Galaxy, List of galaxies | |
NGC 7742 is a face-on unbarred spiral galaxy in the constellation Pegasus.
The galaxy is highly unusual in that it contains a ring but no bar[3]. Typically, bars are needed to produce a ring structure. The bars' gravitational forces move gas to the ends of the bars, where it forms into the rings seen in many barred spiral galaxies. In this galaxy, however, no bar is present, so this mechanism cannot be used to explain the formation of the ring. O. K. Sil'chenko and A. V. Moiseev proposed that the ring was formed partly as the result of a merger event in which a smaller gas-rich dwarf galaxy collided with NGC 7742. As evidence for this, they point to the unusually bright central region, the presence of highly-inclined central gas disk, and the presence of gas that is counterrotating (or rotating in the opposite direction) with respect to the stars[3].
[edit] See also
- NGC 7217 - a face-on spiral galaxy with identical characteristics
- Sombrero Galaxy - a similar galaxy with a dust ring
[edit] References
- ^ a b c d e f g h NASA/IPAC Extragalactic Database. Results for NGC 7742. Retrieved on 2006-08-20.
- ^ Nasa/Fast Facts — Technical information. Results for NGC 7742. Retrieved on 2006-10-12.
- ^ a b O. K. Sil'chenko, A. V. Moiseev (2006). "Nature of Nuclear Rings in Unbarred Galaxies: NGC 7742 and NGC 7217". Astronomical Journal 131: 1366-1346. doi:.
[edit] External links
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