Unformatted text preview: -t a ) is 0.58 days, the length of the primary minimum (t c-t b ) is 0.64 days and the apparent bolometric magnitudes of maximum, primary minimum and secondary minimum are 5.4, 9.20 and 5.44 magnitudes respectively. From this information, and assuming circular orbits, find the a. ratio of stellar masses b. sum of the masses (assume i=90) c. individual masses d. individual radii e. ratio of the effective temperatures of the two stars. Chapter 6 6.4 6.5 6.11 6.14...
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This note was uploaded on 07/28/2011 for the course AST 3018 taught by Professor Lada during the Fall '08 term at University of Florida.
- Fall '08