The wavelength at which maximum energy emission is observed at 40 , 000 K .

Question

Assuming that at the end of the He burning phase of the stellar core (r < R_core) has no H or He or other metals and is composed completely of Carbon, X=Y=0, X_c = 1 ; The envelope above the core has a normal stellar composition ( r > R_core). Calculate the length of time in years that a 1M_sol and 10M_sol star will live on the horizontal branch or the time between the start and end of the He burning phase. Assume that the normal relationship between mass and luminosity holds for horizontal branch stars. Please be as detailed as possible

Answer 1

Question

Chapter 11, Problem 14P

To determine

The wavelength at which maximum energy emission is observed at 40,000 K.

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