NGC 788 | |
---|---|
Observation data ( J2000 epoch) | |
Constellation | Cetus |
Right ascension | 02h 01m 06.46s |
Declination | −06° 48′ 57.15″ |
Redshift | 0.013603±0.000093 |
Heliocentric radial velocity | 4078±28 km/s [1] |
Apparent magnitude (V) | 12.76 |
Characteristics | |
Type | S0 |
Other designations | |
PGC 7656 |
NGC 788 is a lenticular galaxy located in the constellation Cetus. [2] It was discovered in a sky survey by Wilhelm Herschel on September 10, 1785. Studies of NGC 788 indicate that it, while itself being classified as a Seyfert 2, contains an obscured Seyfert 1 nucleus, following the detection of a broad Hα emission line in the polarized flux spectrum. The observation also indicated the lowest radio luminosities observed in an obscured Seyfert 1. [3]
One supernova has been observed in NGC 788: SN 1998dj ( type Ia, mag. 16). [4]
NGC 788 | |
---|---|
Observation data ( J2000 epoch) | |
Constellation | Cetus |
Right ascension | 02h 01m 06.46s |
Declination | −06° 48′ 57.15″ |
Redshift | 0.013603±0.000093 |
Heliocentric radial velocity | 4078±28 km/s [1] |
Apparent magnitude (V) | 12.76 |
Characteristics | |
Type | S0 |
Other designations | |
PGC 7656 |
NGC 788 is a lenticular galaxy located in the constellation Cetus. [2] It was discovered in a sky survey by Wilhelm Herschel on September 10, 1785. Studies of NGC 788 indicate that it, while itself being classified as a Seyfert 2, contains an obscured Seyfert 1 nucleus, following the detection of a broad Hα emission line in the polarized flux spectrum. The observation also indicated the lowest radio luminosities observed in an obscured Seyfert 1. [3]
One supernova has been observed in NGC 788: SN 1998dj ( type Ia, mag. 16). [4]