How to derive angular resolution from bolometric flux, spectral type and temperature

[stuffy]

If we know the bolometric flux, spectral type, and effective temperature of a given star, how can we derive the angular resolution from the information?

This was brought up in class and I've found myself obsessing since I can't figure it out.

 

[meteor]

I've found formula (3) of this page that gives the limb-darkened diameter of a star given its bolometric flux and effective temperature
http://aa.springer.de/papers/8331002/2300619/sc5.htm
Perhaps you know some formula relating the angular resolution with the limb-darkened diameter...

 

[turbo]

If we know the bolometric flux, spectral type, and effective temperature of a given star, how can we derive the angular resolution from the information?

This was brought up in class and I've found myself obsessing since I can't figure it out.

How about using lunar occultations? Here's a link.

www.eso.org/~arichich/[/URL] publications/2001a_a...380..526.pdf