Diffuse interstellar dust emission at wavelengths between 0.5 and 2 mm has been detected by the ARGO 1993 balloon borne telescope. This instrument scanned the Galactic plane in Aquila and several cirrus clouds in Aries, Taurus and Hercules. The data are spatially consistent with the IRAS 100 mu m sky maps, and the spectral behaviour is consistent with a single temperature thermal spectrum with T-d similar to 21 K and a spectral index of emissivity alpha similar to 1.5.
Far infrared multi-frequency observation of interstellar dust clouds / Masi, Silvia; E., Aquilini; A., Boscaleri; DE BERNARDIS, Paolo; DE PETRIS, Marco; M., Gervasi; L., Martinis; V., Natale; P., Palumbo; F., Scaramuzzi. - In: PLANETARY AND SPACE SCIENCE. - ISSN 0032-0633. - STAMPA. - 43:(1995), pp. 1401-1404. [10.1016/0032-0633(95)00075-G]
Far infrared multi-frequency observation of interstellar dust clouds
MASI, Silvia;DE BERNARDIS, Paolo;DE PETRIS, Marco;
1995
Abstract
Diffuse interstellar dust emission at wavelengths between 0.5 and 2 mm has been detected by the ARGO 1993 balloon borne telescope. This instrument scanned the Galactic plane in Aquila and several cirrus clouds in Aries, Taurus and Hercules. The data are spatially consistent with the IRAS 100 mu m sky maps, and the spectral behaviour is consistent with a single temperature thermal spectrum with T-d similar to 21 K and a spectral index of emissivity alpha similar to 1.5.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
