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	- (abs, pdf) Inayoshi et al., Pulsational instability of supergiant protostars: Do they grow supermassive by accretion?
 
	- (abs, pdf) Prestwich et al., Ultra-Luminous X-Ray Sources in the Most Metal Poor Galaxies
 
	- (abs, pdf) Oppenheimer & Schaye, Non-Equilibirum ionisation and cooling of metal-enriched gas in the presence of a photo-ionisation background
 
	 
	
	
	
	
		
		
	- (abs, pdf) Wurster & Thacker, A Comparative Study of AGN Feedback Algorithms
 
	 
	
	
	
	
		
		
	- (abs, pdf) Lebouteiller et al., Chemical enrichment and physical conditions in I Zw 18
 
	 
	
	
	
	
		
		
	- (abs, pdf) Krumholz & Thompson, Numerical Simulations of Radiatively-Driven Dusty Winds
 
	- (abs, pdf) Dekel & Krumholz, Steady Outflows in Giant Clumps of High-z Disk Galaxies during Migration and Growth by Accretion
 
	 
	
	
	
	
		
		
	- (abs, pdf) Scannapieco, Understanding Galaxy Outflows as the Product of Unstable Turbulent Support
 
	- (abs, pdf) Davé et al., The Neutral Hydrogen Content of Galaxies in Cosmological Hydrodynamic Simulations
 
	 
	
	
	
	
		
		
	- (abs, pdf) Bartos et al., G2 can Illuminate the Black Hole Population near the Galactic Center
 
	- (abs, pdf) Huynh et al., Physical Conditions of the Gas in an ALMA [CII]-identified Submillimetre Galaxy at z = 4.44
 
	- (abs, pdf) Baek & Ferrara, Identifying Lyman Alpha Emitters powered by AGNs
 
	 
	
	
	
	
		
		
	- (abs, pdf) MacDonald et al., The extremely low metallicity star SDSS J102915+172927: a subgiant scenario
 
	 
	
	
	
	
		
		
	- (abs, pdf) MacDonald et al., The extremely low metallicity star SDSS J102915+172927: a subgiant scenario
 
	 
	
	
	
	
		
		
	- (abs, pdf) Kannan et al., The MaGICC volume: reproducing statistical properties of high redshift galaxies
 
	- (abs, pdf) Rauch et al., A z=3.045 Lyman alpha emitting halo hosting a QSO and a possible candidate for AGN-triggered star-formation
 
	- (abs, pdf) Shen, The Mass of Quasars
 
	 
	
	
	
	
		
		
	- (abs, pdf) Socrates & Sironi, Photon Feedback: Screening and the Eddington Limit
 
	 
	
	
		
					 
	
		
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