par Ram, Ram;Morbi, Zulfikar;Guo, B;Zhang, Keqing;Bernath, Peter 
;Vander Auwera, Jean ;Johns, John W.C.;Davis, Sumner
Référence The Astrophysical journal. Supplement series, 103, 1, page (247-254)
Publication Publié, 1996
;Vander Auwera, Jean ;Johns, John W.C.;Davis, SumnerRéférence The Astrophysical journal. Supplement series, 103, 1, page (247-254)
Publication Publié, 1996
Article révisé par les pairs
| Résumé : | 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 υ = 0-5. The HF molecule is the most convenient monitor of 19F abundances in cool stars. |
