@article {41808,
	title = {X-ray outburst of RX J0520.5-6932, confirmed as a Be/X-ray binary},
	volume = {4748},
	year = {2013},
	month = {2013/01/1},
	pages = {1},
	abstract = {A Swift observation performed on 2013 January 13 as part of the LMC UV survey (PI: S. Immler) detected the high-mass X-ray binary candidate RX J0520.5-6932 in a moderately bright X-ray outburst. Assuming a power-law spectrum with a photon index of 0.9 and absorption of 10<SUP>21</SUP> cm<SUP>-2</SUP>, we derive a 0.2-12 keV flux of 1.67 {\texttimes} 10<SUP>-12</SUP> erg s<SUP>-1</SUP> cm<SUP>-2</SUP>. This flux is ~25 times higher than measured during a recent XMM-Newton observation (see below).},
	keywords = {Binary, Neutron Star, Optical, Transient, X-Ray},
	url = {https://ui.adsabs.harvard.edu/abs/2013ATel.4748....1V},
	author = {Vasilopoulos, G. and Maggi, P. and Sturm, R. and Haberl, F. and Pietsch, W. and Udalski, A. and Sasaki, M. and Immler, S.}
}
