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Ring Nebula (NGC 6822)

Emission nebula in Barnard's Galaxy From Wikipedia, the free encyclopedia

Ring Nebula (NGC 6822)
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The Ring Nebula in Barnard's Galaxy has the official designation of Hubble 1925 III as it was the third (Roman numeral 3) object recorded in Hubble's 1925 paper, N.G.C. 6822, A Remote Stellar System. It includes areas of bright H II emission. In Paul W. Hodge's 1977 paper it was designated Hodge 4.

Quick facts Emission nebula, Observation data: J2000.0 epoch ...

Its appearance is very similar to the filamentary nebula found in the Large Magellanic Cloud (see Meaburn 1981). It most resembles the circular ring-like nebula N70 in the LMC.

In 1987 this object Hubble III in NGC 6822, was observed with the Manchester Echelle Spectrometer II.[1]

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