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Sh 2-46

From Wikipedia, the free encyclopedia
H II region
Sharpless 2-46
Nebula
Image of Sh 2-46 Nebula
Observation data:epoch
Right ascension18h 06m 6.00s[1]
Declination−14° 08′ 60.0″[1]
Distance6,000 ly   (2,000 pc)
ConstellationSerpens
DesignationsSh 2-46, RCW 158, Gum 80, LBN 58[1]
See also:Lists of nebulae

Sh 2-46 (also known asRCW 158), is anH II region, a glowing cloud of ionized hydrogen gas—located in the southern constellation ofSerpens. Situated approximately 6,000 light-years from Earth, the nebula is notable for its red emission caused by the ionization of hydrogen atoms, energized by the central runaway starHD 165319 (O9.7Ib).[2] It is an isolated nebula positioned above thegalactic plane and containspolycyclic aromatic hydrocarbons (PAHs).[3][4][5] It is located about 3° west of theEagle Nebula (Messier 16) and is part of broader star-forming activity in the region.[6]

Central star

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The primary ionizing source for Sh 2-46 is the massive O-typesupergiant starHD 165319, classified as O9.7Ib. This luminous blue star is arunaway star, believed to have originated in the nearbyEagle Nebula (NGC 6611) but was ejected due to gravitational interactions about 1.8 million years ago. As it travels through Sh 2-46 at high speed, it creates a dynamic environment, including the observedbow shock.[2][3][7][8]

References

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  1. ^abc"Simbad - Object view".simbad.cds.unistra.fr. Retrieved2025-11-16.
  2. ^ab"HD 165319".simbad.cds.unistra.fr. Retrieved2025-11-16.
  3. ^ab"Sh 2-46".galaxymap.org. Retrieved2025-11-16.
  4. ^Giard, M.; Pajot, F.; Lamarre, J. M.; Serra, G.; Caux, E. (May 1989)."The galactic emission in the 3.3 mu-m aromatic feature. I. Observations".Astronomy and Astrophysics.215:92–100.Bibcode:1989A&A...215...92G.ISSN 0004-6361.
  5. ^information@eso.org."There is an impostor in this nebula".www.eso.org. Retrieved2025-11-16.
  6. ^Ritschel, Kevin (2023-10-10)."Explore these three great nebulae".Astronomy Magazine. Retrieved2025-11-16.
  7. ^de Wit, W. J.; Testi, L.; Palla, F.; Vanzi, L.; Zinnecker, H. (October 2004)."The origin of massive O-type field stars. I. A search for clusters".Astronomy and Astrophysics.425 (3):937–948.Bibcode:2004A&A...425..937D.doi:10.1051/0004-6361:20040454.ISSN 0004-6361.
  8. ^Gvaramadze, V. V.; Bomans, D. J. (November 2008)."Search for OB stars running away from young star clusters. I. NGC 6611".Astronomy and Astrophysics.490 (3):1071–1077.Bibcode:2008A&A...490.1071G.doi:10.1051/0004-6361:200810411.ISSN 0004-6361.
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