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		| Paper: | 
		A Possible Extension of the Stellingwerf One-Zone Stellar Model | 
	 
	
		| Volume: | 
		349, Astrophysics of Variable Stars | 
	 
	
		| Page: | 
		313 | 
	 
	
		| Authors: | 
		Pricopi, D. | 
	 
	
	
		| Abstract: | 
		The Stellingwerf one-zone stellar model is being extended by considering a slow and uniform rotation that leads to a very small oblateness of the star. The matter in the core-surrounding shell is supposed to consist of a mixture of ideal gas and radiation. This one-zone stellar pulsation model is proposed as a tool to investigate the linear stability, as well as the factors affecting thermal variation of pulsating stars. Linear and non-linear analyses of the resulting equations are described. | 
	 
	
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