id	author	title	date	pages	extension	mime	words	sentences	flesch	summary	cache	txt
work_cktbuccfhndwlm3imnhbwcxaxy	Daniel Ruschel-Dutra	A mid-IR comparative analysis of the Seyfert galaxies NGC 7213 and NGC 1386	2014	9	.pdf	application/pdf	8561	724	75	T-ReCS high-spatial-resolution data reveal silicate absorption at λ 9.7 µm in the central tens T-ReCS nuclear spectra, we estimate the torus physical properties for both galaxies, finding the torus emission considered it as a continuous density distribution (e.g. Pier & Krolik 1992; Granato, Danese & Franceschini MIR emission of these two galaxies, we used image and spectra PAH emission), Fν (8 µm) and Fν (3.6 µm) are the original flux densities of the 8 and 3.6 µm images and α is the scaling factor for stellar The resulting images are shown in Fig. 1 where we see interstellar emission in NGC the PAH-emitting regions of the host galaxy or being its nucleus. main features of the nuclear spectrum of NGC 1386 are the silicate absorption at 9.7 µm and the [S IV] line, while the host galaxy spectrum shows only an increase in flux towards longer wavelengths due	./cache/work_cktbuccfhndwlm3imnhbwcxaxy.pdf	./txt/work_cktbuccfhndwlm3imnhbwcxaxy.txt