High-Resolution Spectroscopy of Evolved Stars: from ISO to HII/L2

Details High-Resolution Spectroscopy of Evolved Stars: from ISO to HII/L2 High-Resolution Spectroscopy of Evolved Stars: from ISO to HII/L2

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000isass..14...35y&link_type=abstract

The Institute of Space and Astronautical Science Report SP No. 14, p. 35-42.

Astronomy and Astrophysics

Astronomy

Observational Cosmology, Early Universe, Dark Matter

Scientific paper

The observations by the Short-Wavelength Spectrometer onboard the Infrared Space Observatory gave great impetus to the studies of AGB stars. The ISO/SWS has provided high quality, intermediate-resolution spectra covering a broad wavelength range of 2.4-45 micron. These data enable us, for the first time, to perform an extensive study of the outer atmosphere and inner circumstellar regions of AGB stars. Exploration of the undeveloped wavelength regions in the mid- to far-infrared has led to an enormous treasure of dust features. In this review, we particularly focus on the results of the ISO/SWS observations of O-rich objects. We then discuss the possible followup in future missions.

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