The Infrared Spectra of Candidate Materials for Celestial Dust by Laboratory Measurements

Details The Infrared Spectra of Candidate Materials for Celestial Dust by Laboratory Measurements The Infrared Spectra of Candidate Materials for Celestial Dust by Laboratory Measurements

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998isasr.671....1k&link_type=abstract

ISAS Research Note, vol.671, p.1-18

Physics

Ism: Dust, Methods: Laboratory, Infrared: Ism, Techniques: Spectroscopic

Scientific paper

The optical features of various materials interesting in celestial
objects were measured in wavelengths from UV to FIR region. The
unpublished measured spectra of many materials were collected in this
paper. These spectra are used as a clue to identify the observed spectra
and study the evolution of interstellar and/or circumstellar dust.

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