id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2899	Ness, J.-U.	Early Super Soft Source Spectra in RS Oph	2015	4	.pdf	application/pdf	3115	103	60	The line profiles contained clear signs of emission lines in the red wings (figure 5 of Ness et al. 2007) which could either come from residual shock emission or are part of P Cyg profiles. A similar result has been found by (Schönrich & Ness 2008) who show in their figure 1 the evolution of the volume emission measure for various emission lines as a function of their peak formation temperature assuming collisional equi- librium.	cache/app01-2899.pdf	txt/app01-2899.txt