id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2917	Tanabe, K.	Properties of Recurrent Nova T Pyxidis Based on 2011 Outburst	2015	3	.pdf	application/pdf	1784	88	59	2 Summary of Low-resolution Optical Spectroscopy 2.1 Basic properties of T Pyxidis based on pre-2011 outburst As it is mentioned above, T Pyx is a quite unique RN for its very short orbital period (1.83 hour) compared with other RNe. 263 http://dx.doi.org/10.1088/0067-0049/187/2/275 http://dx.doi.org/10.1111/j.1365-2966.2010.17046.x http://dx.doi.org/10.1088/2041-8205/770/2/L33 http://dx.doi.org/10.1017/CBO9780511586491 Introduction Summary of Low-resolution Optical Spectroscopy Basic properties of T Pyxidis based on pre-2011 outburst Spectral classification of novae Spectral evolution of T Pyxidis in its early stage of 2011 outburst Discussion Missing outburst? Is IM Normae a real member of T Pyx subclass? Conclusions	cache/app01-2917.pdf	txt/app01-2917.txt