An editor has determined that sufficient sources exist to establish the subject's notability. (January 2019) |
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.
| Emission nebula | |
|---|---|
| H II region | |
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 |
Image gallery
edit- Image of IC 1318
- On the left image side are the bright North America Nebula (left bright part) with Sadr region (right bright part) in the Cygnus X region, visually interrupted by the Cygnus rift, of the constellation Cygnus, in this X-ray image.
- Butterfly Nebula in narrow band image SHO (north is approximately to the left)
- Image of IC 1318B from astronomer Alpha Zhang
- Amateur image of Sadr (center star) surrounded by IC 1318
- IC1318 by Kasra Karimi
See also
editReferences
edit- 1 2 "IC 1318". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 8 January 2019.