|   | 
				
					
	
		  | 
	 
	
		| Paper: | 
		The White Dwarf Mass Distributions of PCEB  with Different αCE Values | 
	 
	
		| Volume: | 
		469, 18th European White Dwarf Workshop (EUROWD12) | 
	 
	
		| Page: | 
		95 | 
	 
	
		| Authors: | 
		Irawati, P.; Mahasena, P.; Herdiwijaya, D.; Herdiwijaya, D. | 
	 
	
	
		| Abstract: | 
		We report the preliminary results of our population synthesis study 
 for post common-envelope binaries (PCEBs) with a detailed evolutionary 
 process using the STARS code. We concentrate our effort in reproducing 
 the white dwarf mass distribution, and comparing it with the recent 
 observational data from the Sloan Digital Sky Survey Data Release 7 
 for WDMS binaries. We employ the Monte Carlo method to choose the initial 
 parameters of the progenitors (primary mass, mass ratio and orbital period), 
 then we follow the evolution from the zero age main sequence to the end of 
 the common-envelope phase. We include approximate post-Helium flash evolution 
 for primary masses less than 2.0 M☉. We study the effect of 
 using different common envelope ejection efficiency values on the white dwarf 
 mass distribution. In particular, we adopt constant αCE values of 
 0.25, 0.50, and 0.75. The distributions resulting from our population 
 synthesis show a double-peak profile, except for the smallest αCE value. 
 We find that smaller efficiency values significantly affect the post-CE 
 systems with low-mass white dwarf. | 
	 
	
		| 
			
			
		 | 
	 
	
		  | 
	 
 
					 
				 | 
				  |