| NGC 7329 | |
|---|---|
 Hubble Space Telescope image of NGC 7329 | |
| Observation data (J2000 epoch) | |
| Constellation | Tucana |
| Right ascension | 22h 40m 23s |
| Declination | -66°28′44″ |
| Distance | 46,43 ± 3,25 |
| Apparent magnitude (V) | 11.31 |
| Apparent magnitude (B) | 12.51 |
| Surface brightness | 23.36 mag/arcsec2 |
| Characteristics | |
| Type | SBbc |
| Other designations | |
| PGC 69453
ESO 109-12 AM 2236-664 IRAS 22369-6644 | |
NGC 7329 is a large barred spiral galaxy located in the constellation Tucana.[1] NGC 7329 was discovered by British astronomer John Herschel in 1835.[2]
The luminosity class of NGC 7329 is II and it has a broad HI line. To date, 29 non-redshift measurements yield a distance of 44.662 ± 5.536 Mpc (~146 million ly),[3] which is within the Hubble distance range. 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.[4]
- ^ "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-03-22.
- ^ "Natural Sciences program at the Cégep of Valleyfield". astrovalleyfield.ca. Retrieved 2024-03-22.
- ^ "NED Query Results for NGC 7329". ned.ipac.caltech.edu. Retrieved 2024-03-22.
- ^ "SN 2006bh | Transient Name Server". www.wis-tns.org. Retrieved 2024-03-22.