Sh 2-9 Explained

Sh2-9
Type:Emission
Epoch:J2000.0
Ra:16h 21m 11.31s
Dec:-25d 35m 34.05
Dist Ly:568
Dist Pc:174
Appmag V:2.89
Constellation:Scorpius
Names:Gum 65, LBN 1101, HD 147165, IRAS 16181-2528

Sh 2-9, also known as Gum 65, is combination emission and reflection nebula in the Scorpius constellation, surrounding the multiple star system Sigma Scorpii. Sigma Scorpii is 1° to the northwest of Messier 4,[1] and the nebula can be easily seen with small telescopes.

Sharpless 9 is a red emission nebula that surrounds the star Sigma Scorpii.[2] It is thought the star Sigma Scorpii, a variable giant star, is ionizing this region.[3] It is also recorded as reflection nebula C130.

This region is noted as both an emission and reflection nebula, although sometimes only one aspect is noted.[4]

The magnitude 1.1 Antares is 2° to the southeast of this nebula.

One of strongest 2.3 GHz sources in the region coincides with Sharpless 9.[5]

There is a radio source on the edge, and it has been proposed that this is because there is a collision between this nebula and the dark nebula Kh 527.

Catalogs

Examples:

External links

Notes and References

  1. Web site: SH2-9 . Sharpless Catalog . SharplessCatalog.Com.
  2. Book: Structures in Space: Hidden Secrets of the Deep Sky. Abrams. Bernard. Stecker. Michael. 2012-12-06. Springer Science & Business Media. 9781447104414. en.
  3. Web site: The Gum Catalog. galaxymap.org. 2019-10-30.
  4. Book: Gilmour, Jess K.. The Practical Astronomer's Deep-sky Companion. 2003. Springer Science & Business Media. 9781852334741. en.
  5. etal . E. E. Baart . A 2.3 GHz radio continuum map of the upper Scorpio region . Astronomy and Astrophysics . Dec 1980 . 92 . 156 . 1980A&A....92..156B .