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- W1590659444 abstract "The study of dust in space was for a long time hampered by the lack of resolution and wavelength coverage in the infrared. The launch of the Infrared Space Observatory (ISO) changed this dramatically. Its unprecedented wavelength range (2.4 - 200 μm) together with its relatively high spectral resolution (λ/Δλ = 2000–150) made this instrument ideal to study dust in space. Many new dust species have been found, in particular of oxygen-rich species. The quality of the data allows a detailed mineralogy of individual species. The ISO database can be used to carry out an inventory of the occurrence of dust species in various circumstellar and interstellar environments. The picture that emerges is that of a very rich circumstellar dust mineralogy, while the interstellar medium shows only a limited amount of species. We present an overview of this inventory, as well as of the mineralogy of the dust species found. The implications for our understanding of dust processing in different astrophysical environments are also discussed." @default.
- W1590659444 created "2016-06-24" @default.
- W1590659444 creator A5034532818 @default.
- W1590659444 creator A5060973665 @default.
- W1590659444 date "2003-01-01" @default.
- W1590659444 modified "2023-10-15" @default.
- W1590659444 title "The Mineralogy of Interstellar and Circumstellar Dust" @default.
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