|   | 
				
					
	
		  | 
	 
	
		| Paper: | 
		Sagittarius Dwarf Spheroidal and M54 in the 1612 MHz OH Line | 
	 
	
		| Volume: | 
		497, Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time | 
	 
	
		| Page: | 
		501 | 
	 
	
		| Authors: | 
		Sjouwerman, L. O.; Claussen, M. J. | 
	 
	
	
		| Abstract: | 
		We have observed the M 54 region in the Sagittarius Dwarf Spheroidal
 galaxy with the VLA for 1612 MHz OH emission in an attempt to detect 
 OH/IR stars outside the Galaxy and LMC. With an rms noise of 
 ∼1 mJy/beam in a ∼1 km s-1 channel, we do not, however, 
 detect any line sources. | 
	 
	
		| 
			
			
		 | 
	 
	
		  | 
	 
 
					 
				 | 
				  |