Infrared Spectra of Hot HF and DF

Details Infrared Spectra of Hot HF and DF Infrared Spectra of Hot HF and DF

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apjs..103..247r&link_type=abstract

Astrophysical Journal Supplement v.103, p.247

Astronomy and Astrophysics

Astronomy

19

Line: Identification, Methods: Laboratory, Molecular Processes, Stars: Abundances

Scientific paper

New Fourier transform emission measurements were obtained for HF and DF at a temperature of 2300 °C. Both pure rotation and vibration-rotation lines were measured with a precision of about 0.0005 cm-1. These new lines were combined with previously measured data to give improved rotational constants for the vibrational levels V = 0-5. The HF molecule is the most convenient monitor of 19F abundances in cool stars.

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