NGC 3817
Appearance
From Wikipedia, the free encyclopedia
Galaxy in the Virgo constellation
NGC 3817 | |
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Observation data (J2000 epoch) | |
Right ascension | 11h 41m 52.9487s |
Declination | +10° 18′ 15.7838″ |
Redshift | 0.02026 |
Characteristics | |
Type | SB (R) c |
Notable features | LINER-type Active Galaxy Nucleus |
Other designations | |
GSC 04937-00483, LEDA 36304, UGCA 243 |
NGC 3817 is a barred spiral galaxy located approximately 91.7 million light-years away in the constellation Virgo. It was discovered by the German-British astronomer William Herschel on March 15, 1784, using his telescope in Slough, England. Classified as a LINER-type Active Galactic Nucleus (AGN), NGC 3817 exhibits low-ionization nuclear emission lines from its core. With an apparent magnitude of 14.4, the galaxy features a faint ring structure and loosely wound spiral arms.[1]
References
[edit]- ^ "NGC 3817 - Lenticular Galaxy in Virgo | TheSkyLive.com". theskylive.com. Retrieved 2024-11-01.
This galaxy-related article is a stub. You can help Wikipedia by expanding it. |
New General Catalogue 3500 to 3999 | |
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