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Q2. Spectroscopic parallax. (Apparent)
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magnitude
= 5.4 for an O6 V star. How far
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away
is it? First need to get an absolute
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magnitude. Can estimate it several ways
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(H-R
diagrams, mass-luminosity relation).
I
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used
M = -5.6. So:
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d (pc) = 10 (m-M+5)/5 = 103.2 = 1585 parsecs
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