Dust enshrouded star-forming activity in Arp 299

We present mid-infrared spectro-imaging (5-16 μm) observations of the infrared luminous interacting system Arp 299 (= Mrk 171 = IC 694+NGC 3690) obtained with the ISOCAM instrument aboard ISO. Our observations show that nearly 40% of the total emission at 7 and 15 μm is diffuse, originating from the...

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Detalles Bibliográficos
Autores principales:	Gallais, P., Charmandaris, V., Le Floc'h, E., Mirabel, I.F., Sauvage, M., Vigroux, L., Laurent, O.
Formato:	JOUR
Materias:	Galaxies: individual: Arp 299 Galaxies: individual: Mrk 171 Galaxies: interactions Galaxies: starburst Infrared: ISM Stars: formation Atmospheric optics Computer simulation Cosmic rays Data reduction Extraterrestrial atmospheres Galaxies Infrared imaging Infrared radiation Infrared spectroscopy Hot dust Mid infrared spectro imaging Star forming activity Stars Unidentified infrared bands Astrophysics
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00046361_v414_n3_p845_Gallais
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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