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IC 2118

Coordinates:Sky map05h04m54s,−07° 15′ 00″
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IC 2118
Reflection nebula
IC 2118
Observation data:J2000epoch
Right ascension05h02m00.0s[citation needed]
Declination−07° 54′ 00″[citation needed]
Distance1,000[citation needed]ly
Apparent magnitude(V)13[citation needed]
Apparent dimensions (V)3 ×1°[citation needed]
ConstellationEridanus
DesignationsWitch Head Nebula, Cederblad 41[citation needed]
See also:Lists of nebulae

IC 2118(also known asWitch Head Nebuladue to its shape) is an extremely faintreflection nebulabelieved to be an ancient supernova remnant or gas cloud illuminated by nearbysupergiantstarRigelin the constellation ofOrion.The nebula lies in theEridanusConstellation,[1]about 900light-yearsfromEarth.The nature of the dust particles, reflecting blue light better than red, is a factor in giving the Witch Head its blue color. Radio observations show substantial carbon monoxide emission throughout parts of IC 2118, an indicator of the presence of molecular clouds and star formation in the nebula. In fact candidates for pre-main sequence stars and some classicT-Tauri starshave been found deep within the nebula.[2]

The molecular clouds of IC 2118 are probably juxtaposed to the outer boundaries of the vastOrion-Eridanus bubble,a giant supershell of molecular hydrogen blown by the high mass stars of theOrion OB1 association.As the supershell expands into the interstellar medium, favorable circumstances for star formation occur. IC 2118 is located in one such area. The wind blown appearance and cometary shape of the bright reflection nebula is highly suggestive of a strong association with the high mass luminous stars of Orion OB1. The fact that the heads of the cometary clouds of IC2118 point northeast towards the association is strong support of that relationship.

See also

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References

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  1. ^"Witch Head Nebula".NASA.Archivedfrom the original on 2023-06-22.
  2. ^Kun; Prusti, T.; Nikolić, S.; Johansson, L. E. B.; Walton, N. A. (2004). "The IC 2118 association: New T Tauri stars in high-latitude molecular clouds".Astronomy and Astrophysics.418(1): 89–98.arXiv:astro-ph/0402353.Bibcode:2004A&A...418...89K.doi:10.1051/0004-6361:20034510.S2CID15970267.
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