id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
app01-2908	Kajikawa, T.; Arai, A.; Nagashima, M.; Kawakita, H.; Yamanaka, M.; Kawabata, K.; Kiyota, S.	Line Evolution of the Nova V5587 Sgr from Early to Nebula Phase	2015	4	.pdf	application/pdf	2052	124	76	The light curve of V5587 Sgr is quite similar to that of the “Jitter”class nova PW Vul as shown Figure 1 (Schwarz et al. 1997, and references therein). 242 Acta Polytechnica CTU Proceedings 2(1): 242–245, 2015 242 doi: 10.14311/APP.2015.02.0242 Line Evolution of the Nova V5587 Sgr from Early to Nebula Phase T. Kajikawa1, A. Arai1,2, M. Nagashima1, H. Kawakita1, M. Yamanaka3,4,5, K. Kawabata3, S. Kiyota6 1Kyoto Sangyo University, Koyama Astronomical Observatory 2University of Hyogo, Nishi-Harima Astronomical Observatory 3Hiroshima University 4Kyoto University 5Konan University 6VSOLJ Corresponding author: kajikawat8@gmail.com	cache/app01-2908.pdf	txt/app01-2908.txt