- #1
Brewer
- 212
- 0
How do I go about working out the radius of a star when I have the bolometric flux, the wavelength of the peak flux of its spectrum, and its parallax?
I've also calculated the temperature of its photosphere (Wein's law right?).
Or is it more to do with the parallax?
I've also calculated the temperature of its photosphere (Wein's law right?).
Or is it more to do with the parallax?