Clamshell Nebula
| Emission nebula | |
|---|---|
| H II region | |
| Observation data: epoch | |
| Right ascension | 21h 18m 30s |
| Declination | +43° 56' 00"[1] |
| Distance | ~2,200[2] ly |
| Apparent diameter | 3°[3] |
| Constellation | Cygnus |
| Designations | Sh 2-119, LBN 391, [GS55] 240[4] |
The Clamshell Nebula (also known as Sh 2-119) is an emission nebula and star-forming region located in the constellation Cygnus.[5]
The Clamshell Nebula was discovered in the early 1950s by Grigory Abramovich Shajn and Vera Fedorovna Gaze while conducting a photographic survey, and they named it Gaze+Shajn [GS55] 240. Stewart Sharpless would survey the region of the sky in more detail in 1959, revealing that the nebula was much more extensive than originally though. He included it in his sharpless catalog, giving it the designation Sh 2-119.[1]
The nebula surrounds blue giant 68 Cygni. The nebula contains multiple dust lanes and bok globules.[6] 68 Cygni is the primary source of ionization within the nebula. The structure of the nebula is that of a Strömgren sphere, and is divided into an eastern and western section, with 68 Cygni between the two. These two sections are the reason for the 'clamshell' name.[2][7] It was originally proposed that this nebula was formed from 68 Cygni's stellar wind. Instead, the stellar wind is likely due to the star's high velocity through space, forming a bow shock.[8] The planetary nebula PK 87-3.1 is located within the nebula.[3] and open cluster NGC 7044 is located nearby.[9]
References
- ^ a b "Clamshell Nebula (Sh 2-119)". Deep Sky Corner.
- ^ a b Dani, Gerd (January 26, 2024). "Exploring the Clamshell Nebula in Cygnus". FreeAstroScience.
- ^ a b "SH2-119 (Sharpless 119 )". Sharpless Catalog.
- ^ "LBN 087.23-03.80". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2026-07-18.
- ^ "Sh2-119 The Clamshell Nebula".
- ^ "Sh2-119 Clamshell nebula". Caprile Observatory. March 13, 2022.
- ^ Génier, Ryan. "A clam in Cygnus". Astronomy.com.
- ^ Wisotzki, L.; Wendker, H. J. (1989). "Is HS 240 an interstellar bubble?". Astronomy and Astrophysics. 221: 311. Bibcode:1989A&A...221..311W.
- ^ Brecher, Ron. "Sh2-119". Astro Doc.
Content Disclaimer
Informasi ini disarikan dari Wikipedia dan disajikan kembali untuk tujuan edukasi. Konten tersedia di bawah lisensi CC BY-SA 3.0. Kami tidak bertanggung jawab atas ketidakakuratan data yang bersumber dari kontribusi publik tersebut.
- The information displayed on this website is sourced in part or in whole from Wikipedia and has been adapted for the purpose of restating it. We strive to provide accurate and relevant information, however:
- There is no guarantee of absolute accuracy. Wikipedia is an open, collaborative project that can be edited by anyone, so information is subject to change.
- It is not intended to constitute professional advice. The content displayed is for informational and educational purposes only. For important decisions (e.g., medical, legal, or financial), please consult a professional.
- Content copyright. Wikipedia is licensed under the Creative Commons Attribution-ShareAlike License (CC BY-SA). This means that content may be reused with appropriate attribution and shared under a similar license.
- Responsible use. Any risk arising from the use of information from this website is entirely the responsibility of the user.