id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2854	Balman, S.	Inner Disk Structure of Dwarf Novae in the Light of X-Ray Observations	2015	7	.pdf	application/pdf	4927	187	62	On the other hand, some DN show increased level of X-ray emission (GW Lib & U Gem: Byckling et al. 2009, Guver et al. 2006). During the outburst stage, DN X-ray spec- tra differ from the quiescence since the accretion rates are higher (about two orders of magnitude), the BL is expected to be optically thick emitting EUV/soft X- rays (Lasota 2001, see the X-ray review in Kuulkers et al. 2006).	cache/app01-2854.pdf	txt/app01-2854.txt