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DWB 169 - Nebula
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DWB 169

description DWB 169 Overview

DWB 169 is a catalogued Galactic emission nebula in the Cygnus X star-forming region of the Milky Way. The designation comes from the DWB radio-continuum survey, which identified nebular sources in this part of the Galaxy in 1969. It belongs to the H II-region category, in which ionized hydrogen around young stars helps researchers study processes linked to star formation. The entry is for readers interested in Galactic nebulae, radio surveys, and Cygnus X.

help DWB 169 FAQ

What is DWB 169?

DWB 169 is a catalogued Galactic emission nebula in the Cygnus X star-forming region. It belongs to the H II-region category.

What does the DWB designation refer to?

The designation comes from the DWB radio-continuum survey. That survey identified nebular sources in this part of the Galaxy in 1969.

Where is DWB 169 located?

DWB 169 is located in the Cygnus X star-forming region of the Milky Way. Cygnus X is a major area of stellar birth and ionized gas.

What is an H II region?

An H II region is a cloud of ionized hydrogen associated with hot young stars. DWB 169 is classified as a Galactic emission nebula of this type.

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