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