Step 1: Understanding the Concept
Wien's displacement law says \(\lambda_mT=b\), a constant. A hotter star radiates its peak energy at a shorter wavelength.
Step 2: Write for both stars
\[ \lambda_AT_A=\lambda_BT_B\Rightarrow\frac{T_A}{T_B}=\frac{\lambda_B}{\lambda_A} \]
Step 3: Substitute
\[ \frac{T_A}{T_B}=\frac{5.2\times10^{-7}}{3.9\times10^{-7}}=\frac{52}{39}=\frac43 \]
Step 4: Check the options
Star A has the shorter wavelength, so it is the hotter one and the ratio must be greater than 1. That rules out 2:3 and 3:4. The value 3:2 would need a wavelength ratio of 1.5, which does not match 5.2/3.9. So the answer is 4:3, option (D).
Final Answer:
The temperature ratio equals the inverse wavelength ratio, 5.2 over 3.9, which is 4 to 3, option (D).
\[ \boxed{4:3} \]