Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996dln.........46.&link_type=abstract
Daresbury Laboratory: Newsletter on Analysis of Astronomical Spectra, p. 46
Astronomy and Astrophysics
Astrophysics
Atmospheric Chemistry, Infrared Space Observatory (Iso), Stellar Evolution, Stellar Mass, Dust, Molecular Gases, Molecules, Space Missions, Astrophysics, Stellar Envelopes, Infrared Spectra
Scientific paper
Late stages of evolution of low- and high-mass stars are characterized by very different circumstellar environments, but observations of these objects at optical, infrared and millimetre wavelengths often reveal the presence of the same type of solid compounds and molecular species. The aim of this workshop is to gather scientists working on late stages of stellar evolution to discuss the nature and the role of dust and molecules in evolved objects and to address and answer fundamental questions such as how the same type of solid compounds and molecular species can form in very different astrophysical environments. A large fraction of the Infrared Space Observatory ISO mission is dedicated to the study of evolved objects and the workshop will be an opportunity to present new and exciting ISO results on circumstellar matter related to late stages of stellar evolution.
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