Far infrared multi-frequency observation of interstellar dust clouds

S. Masi, E. Aquilini, A. Boscaleri, P. de Bernardis, M. De Petris, M. Gervasi, L. Martinis, V. Natale, P. Palumbo, F. Scaramuzzi

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Abstract

Diffuse interstellar dust emission at wavelengths between 0.5 and 2 mm has been detected by the ARGO 1993 balloon borne telescope. The 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 μm sky maps, and the spectral behaviour is consistent with a single temperature thennal spectrum with Td∼ 21 K and a spectral index of emissivity α ∼ 1.5. © 1995.
Original languageEnglish
Pages (from-to)1401 - 1404
Number of pages4
JournalPlanetary and Space Science
Volume43
Issue number10-11
DOIs
Publication statusPublished - 1995
Externally publishedYes

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All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Masi, S., Aquilini, E., Boscaleri, A., de Bernardis, P., De Petris, M., Gervasi, M., ... Scaramuzzi, F. (1995). Far infrared multi-frequency observation of interstellar dust clouds. Planetary and Space Science, 43(10-11), 1401 - 1404. https://doi.org/10.1016/0032-0633(95)00075-G