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The best single wavelength band for mapping out the spiral arm structure of the Milky Way Galaxy is the infrared band, particularly around 2.2 micrometers (K-band). Infrared observations can penetrate dust clouds that obscure visible light, allowing astronomers to see the underlying structure of the spiral arms and the distribution of stars and gas within them. This capability makes infrared a crucial tool in understanding the dynamics and morphology of our galaxy.

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1mo ago

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