id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2822	Sion, E. M.; Godon, P.	White Dwarfs in Cataclysmic Variables: An Update	2015	6	.pdf	application/pdf	3697	128	65	In section 2, our FUV analysis techniques are briefly summarized, sec- tion 3 we address how the revised (shorter) distance to SS Cygni affects the results of our analysis of the FUSE + HST STIS spectra of SS Cygni by Sion et al. (2010), in section 4 we tabulate and display the current distribution of CVWD surface temperatures versus or- bital period and in the final section, we include some remarks on new HST spectra of the recurrent nova T Pyxidis. An obvious question is: How does the new, shorter dis- tance affect the analysis of Sion et al. (2010) regarding their detection of the WD during quiescence and their derivation of the WD’s surface temperature from the modeling of FUSE + HST STIS spectra? To answer this question, we have carried out model fits using the new distance in the range of 114 pc to 120 pc.	cache/app01-2822.pdf	txt/app01-2822.txt