id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2826	Kononov, D. A.; Bisikalo, D. V.; Puzin, V. B.; Zhilkin, A. G.	Transient Processes in a Binary System with a White Dwarf	2015	4	.pdf	application/pdf	2679	122	64	In Section 3, based on the results of gas dynamic simulations we consider a physical model of the formation of the humps in orbital light curves of WZ Sge stars. Another model, mentioned, for instance, by Wolf (1998) and Silvestri et al., (2012) supposes that the stream from the inner Lagrangian point may over- flow the disk after it ricochets on the disk rim and forms an additional hot spot at the opposite side of the disk, i.e. two hot spots give two humps in the light curve.	cache/app01-2826.pdf	txt/app01-2826.txt