id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
4m90dv15v60	Rashi Talwar	Stellar Neutron Sources and s-Process in Massive Stars	2015		.txt	text/plain	529	22	55	Hence, the recommended 22Ne(&alpha,n) + 22Ne(&alpha,&gamma) rates, from the present work, strongly favour the reduction of s-process over-abundances associated with massive stars as well as AGB stars of intermediate initial mass. and Bisterzo et al. rates and by a factor of 3 above NACRE rate.	cache/4m90dv15v60.txt	txt/4m90dv15v60.txt