Wiki Article
IC 1318
Nguồn dữ liệu từ Wikipedia, hiển thị bởi DefZone.Net
 | An editor has determined that sufficient sources exist to establish the subject's notability. (January 2019) |
| Emission nebula | |
|---|---|
| H II region | |
.jpg) Image of IC 1318 with Crescent Nebula in the lower right side and Gamma Cygni star in the upper left side as well as some other nebulous regions | |
| Observation data: J2000 epoch | |
| Right ascension | 20h 16m 48.0s[1] |
| Declination | +41° 57′ 24″[1] |
| Constellation | Cygnus |
| Designations | IC 1318, Gamma Cyg Nebula, Sadr Region |
IC 1318 (also known as Gamma Cygni Nebula) is the diffuse emission nebula and a H II region surrounding the star Sadr (γ Cygni) at the center of Cygnus's cross thus getting a nickname Sadr Region. The Sadr Region is one of the surrounding nebulous regions; others include the Butterfly Nebula and the Crescent Nebula. It contains many dark nebulae in addition to the emission diffuse nebulae.
See also
[edit]References
[edit]- ^ a b "IC 1318". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 January 2019.
 | This nebula-related article is a stub. You can help Wikipedia by adding missing information. |