SpS1-Laboratory spectroscopy of small molecules

Details SpS1-Laboratory spectroscopy of small molecules SpS1-Laboratory spectroscopy of small molecules

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..541b&link_type=abstract

Highlights of Astronomy, Volume 15, p. 541-542

Astronomy and Astrophysics

Astronomy

Scientific paper

This contribution focuses on the study of ‘cool’ sources with surface temperatures in the range of about 500-4000 K. In this temperature range spectra are dominated by strong molecular absorption and the tools of modern chemical physics can be applied to compute the molecular opacities needed to simulate the observed spectral energy distributions. (See Bernath (2005) for an introduction to molecular spectroscopy including line intensities and Bernath (2009) for a recent astronomical review article.)

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