id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2888	De Bianchi, S.; Braga, V. F.; Gaudenzi, S.	The Role of Magnetic Field for Quiescence-Outburst Models in CVs	2015	5	.pdf	application/pdf	3398	135	54	For this process to occur, an intense magnetic field 106−108 G is required; primaries with such fields do exist in Interme- diate polars (IPs) and Polars that owe their properties to the very primary magnetic field (Patterson 1994). 192 Acta Polytechnica CTU Proceedings 2(1): 192–196, 2015 192 doi: 10.14311/APP.2015.02.0192 The Role of Magnetic Field for Quiescence-Outburst Models in CVs S. De Bianchi1,2, V. F. Braga3, S. Gaudenzi1 1Dept. of Physics, Università degli Studi di Roma ”La Sapienza”, Piazzale A. Moro 5, 00185 Rome, Italy 2École Normale Supérieure, CNRS-UMR 8547, Rue d’Ulm 45, 75005 Paris, France 3Dept. of Physics, Università Tor Vergata, Via della Ricerca Scientifica 1, 00133 Rome, Italy Corresponding author:	cache/app01-2888.pdf	txt/app01-2888.txt