double line The velocity curve spectroscopic binary is shown in the sketch. The system is viewed edge-on, i.e., with an inclination angle of i = 90°, so that the maximum possible Doppler shifts for this system are observed. for a 400 So = U, Ani 300 200 no - V Ain i 100 -100 -200 -300 400 • 1 2 3 . S 6 7 8 10 Time (days) Find the mass ratio, m1/m2, of the stars. Express your answer as a fraction like a/b Doppler Velocity
double line The velocity curve spectroscopic binary is shown in the sketch. The system is viewed edge-on, i.e., with an inclination angle of i = 90°, so that the maximum possible Doppler shifts for this system are observed. for a 400 So = U, Ani 300 200 no - V Ain i 100 -100 -200 -300 400 • 1 2 3 . S 6 7 8 10 Time (days) Find the mass ratio, m1/m2, of the stars. Express your answer as a fraction like a/b Doppler Velocity
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Transcribed Image Text:double line
The velocity curve
spectroscopic binary is shown in the sketch.
The system is viewed edge-on, i.e., with an
inclination angle of i = 90°, so that the
maximum possible Doppler shifts for this
system are observed.
for a
400
So = U, Ani
300
200
no - V Ain i
100
-100
-200
-300
400
• 1 2 3 .
S 6 7 8
10
Time (days)
Find the mass ratio, m1/m2, of the stars.
Express your answer as a fraction like a/b
Doppler Velocity
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