id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2850	Scaringi, S.	Broad-Band Variability in Accreting Compact Objects	2015	4	.pdf	application/pdf	2787	120	58	As a result, X-ray binaries emit most of their radiation at X-ray wavelengths, as opposed to cataclysmic variables which emit mostly at optical/ultraviolet wavelengths. A natural explanation for hard lags in XRBs comes from the fluctuating accre- tion disk model (see Arevalo & Uttley 2006 and ref- erences therin), where the coupling of fluctuations in the mass-transfer rate at different accretion disk radii is responsible for the observed variability.	cache/app01-2850.pdf	txt/app01-2850.txt