What lies hidden in the ISO archive on solid-state dust features?

Details What lies hidden in the ISO archive on solid-state dust features? What lies hidden in the ISO archive on solid-state dust features?

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511...55j&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

Scientific paper

The Infrared Space Observatory has revolutionized the study of solid-state interstellar matter whether this refers to molecular ices, carbonaceous dust or oxides (silicates and others). Promising studies have been initiated on the formation and processing of dust in the cycle of interstellar matter. Dust features are also becoming a powerful and, in a way, unique tool to quantify the evolutionary stage of astronomical objects. This paper provides a short overview of this rich field, underlining the importance of a full, thoughtful and organised exploitation of the ISO data archive in close connection with a large field of activities: laboratory experiments, theory and radiative transfer modelling.

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