The Milky Way: A structural overview
Structure of the Milky Way Disk Density distribution roughly follows an exponential in R and z:!",$=! P&RS⁄T!&RU⁄T" where ℎ %andℎ &are the radial scale length and vertical scale height, respectively. Radial scale length ℎ %≈3 kpc (estimates range 2.5 –3.5 kpc) Vertical scale height ℎ &turns out to have a complex dependency on ................
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