id	author	title	date	pages	extension	mime	words	sentence	flesch	summary	cache	txt
bibechana-20960	Gautam, A K; Aryal, B	Study of far infrared cavity around a post AGB star under IRAS survey at galactic latitude -3°	2018	8	.pdf	application/pdf	3395	175	66	According to Schnee et al. (2005)[8], dust color temperature of the emission at a wavelength λi is given by �� � ��� � ��.�����)� (1) where , R = F(60 μm)F(100 μm) Fig. 1: (a) & (b) IRAS 60 μm and 100 μm far infrared image of the core region of AGB 08-36 centered at R.A. (J2000)= 08h 04m 07.21s and Dec.(J2000) In this article, we have calculated dust color temperature, dust mass and size.	cache/bibechana-20960.pdf	txt/bibechana-20960.txt