id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
ap-1310	Giovannelli, F.; Sabau-Graziati, L.	X-ray Transient Sources (Multifrequency Laboratories) The Case of the Prototype A0535+26/HDE 245770	2011	12	.pdf	application/pdf	6793	290	67	The shape and intensity of X-ray outbursts are dependent on the strength of the activity of the primary. Thus the passage of the neutron star at the periastron occurs with a periodicity of 110.856 ± 0.02 days and the different kinds of X-ray outbursts of A0535+26 — following the definitions reported in the review by Giovannelli & Sabau-Graziati (1992) — occur just after ∼ 8 days.	cache/ap-1310.pdf	txt/ap-1310.txt