Infrared spectroscopy of star-forming regions - Some recent results of interest

Details Infrared spectroscopy of star-forming regions - Some recent results of interest Infrared spectroscopy of star-forming regions - Some recent results of interest

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95..556g&link_type=abstract

(Astronomical Society of the Pacific, Symposium on the Renaissance in High-Resolution Spectroscopy - New Techniques, New Frontie

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Infrared Astronomy, Interstellar Matter, Protostars, Stellar Evolution, Carbon Monoxide, Cosmic Dust, High Resolution, Hydrogen Clouds

Scientific paper

A brief summary of the major events in star formation is given. Three
infrared spectroscopic phenomena currently being studied in star-forming
regions are discussed: atomic hydrogen recombination lines in
protostars, molecular hydrogen emission lines in shocked clouds, and
solid-state absorption features due to molecules on grain mantles.

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