-0.5 = Compute the Oort constants A and B for Keplerian rotation: 0(R) Oo (R/Ro) in terms of eo and Ro. If Keplerian rotation described the rotation of the Milky Way near the Sun, what would the numerical value of A and B (in kms¯¹ kpc¯¹) be and how does this

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Problem 1: (
Compute the Oort constants A and B for Keplerian rotation: 0(R) = O, (R/Ro)
terms of O, and Ro. If Keplerian rotation described the rotation of the Milky Way near the
Sun, what would the numerical value of A and B (in kms-1 kpc-1) be and how does this
-0.5
in
compare to the observed values?
Transcribed Image Text:Problem 1: ( Compute the Oort constants A and B for Keplerian rotation: 0(R) = O, (R/Ro) terms of O, and Ro. If Keplerian rotation described the rotation of the Milky Way near the Sun, what would the numerical value of A and B (in kms-1 kpc-1) be and how does this -0.5 in compare to the observed values?
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