id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2841	Meintjes, P. J.; Odendaal, A.; van Heerden, H.	AE Aquarii: A Short Review	2015	4	.pdf	application/pdf	2911	111	63	The low accretion rate of the white dwarf in AE Aquarii (Ṁ∗ ∼ 1014 g s−1) compared to the mass transfer rate deduced from the UV emission line spectra (Ṁ2 ∼ 1017 g s−1) implies that the white dwarf in AE Aquarii is in a super-propeller (ejector) state (Bisikalo & Zhilkin 2012; Ikhsanov & Beskrovnaya 2012). The low accretion in comparison to the mass trans- fer α = Ṁ∗/Ṁ2 ∼ 0.1% may indicate that the white dwarf in AE Aquarii is currently in a super-propeller (Bisikalo & Zhilkin 2012) or ejector phase (Ikhsanov & Beskrovnaya 2012) and that the white dwarf in AE Aquarii may exhibit the same properties as a spun-up radio pulsar (e.g Ikhsanov & Bierman 2006).	cache/app01-2841.pdf	txt/app01-2841.txt