NGC 767
- العربية
- Azərbaycanca
- Беларуская
- Bosanski
- Deutsch
- Ελληνικά
- Esperanto
- Euskara
- Français
- Hrvatski
- Italiano
- Қазақша
- Lëtzebuergesch
- Македонски
- مصرى
- Nederlands
- Нохчийн
- Oʻzbekcha / ўзбекча
- Polski
- Português
- Română
- Русский
- Slovenčina
- Српски / srpski
- Srpskohrvatski / српскохрватски
- Татарча / tatarça
- Türkçe
- Українська
- Zazaki
- 中文
Appearance
From Wikipedia, the free encyclopedia
Galaxy located in the constellation Cetus
NGC 767 | |
---|---|
SDSS image of NGC 767 | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 01h 58m 50.822s |
Declination | −09° 35′ 13.61″ |
Redshift | 0.01805[1] |
Heliocentric radial velocity | 5362 km/s[1] |
Distance | 246.5 ± 17.3 Mly (75.58 ± 5.3 Mpc)[2] |
Apparent magnitude (B) | 14[1] |
Characteristics | |
Type | SBb pec?[2] |
Other designations | |
MCG -02-06-010, PGC 7483[1] |
NGC 767 is a barred spiral galaxy located in the constellation Cetus about 241 million light years from the Milky Way. It was discovered by the American astronomer Francis Leavenworth in 1886.[3] [4] [5]
One supernova has been observed in NGC 767: SN 2019lre (type II, mag. 19.2).[6]
See also
[edit ]References
[edit ]- ^ a b c d "NGC 767". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020年05月24日.
- ^ a b "Results for object NGC 0767 (NGC 767)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020年05月24日.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020年03月30日.
- ^ "Revised NGC Data for NGC 767". spider.seds.org. Retrieved 2020年03月30日.
- ^ Ford, Dominic. "The galaxy NGC 767 - In-The-Sky.org". in-the-sky.org. Retrieved 2020年03月30日.
- ^ "SN 2019lre". Transient Name Server. IAU . Retrieved 6 September 2024.
External links
[edit ]- Media related to NGC 767 at Wikimedia Commons
Stub icon
This spiral galaxy article is a stub. You can help Wikipedia by expanding it.
Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_767&oldid=1244365101"