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RCW 122 - Nebula
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RCW 122

description RCW 122 Overview

RCW 122 is a southern Milky Way H-alpha emission region listed in the 1960 RCW catalog, which mapped nebulae from Mount Stromlo data.

help RCW 122 FAQ

What is RCW 122?

RCW 122 is an H-alpha emission region in the southern Milky Way. It is listed in the RCW catalog, a 1960 survey based on observations from Mount Stromlo.

What does the RCW designation mean?

RCW refers to the catalog compiled from Mount Stromlo observations of southern emission nebulae. The number 122 identifies this particular entry in that catalog.

What kind of nebula is RCW 122?

RCW 122 is described as an emission region, meaning glowing hydrogen produces strong H-alpha light. It is located in the southern part of the Milky Way.

Why do astronomers use H-alpha surveys for regions like RCW 122?

H-alpha surveys reveal ionized hydrogen, which helps astronomers locate star-forming and excited gas regions. The RCW catalog made such southern Milky Way features easier to identify and compare.

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