The ultraviolet NH bands as indicators of the nitrogen abundance in atmospheres of cool stars.

Details The ultraviolet NH bands as indicators of the nitrogen abundance in atmospheres of cool stars. The ultraviolet NH bands as indicators of the nitrogen abundance in atmospheres of cool stars.

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998kfnt...14..257y&link_type=abstract

Kinematika Fiz. Nebesn. Tel, Tom 14, No. 3, p. 257 - 267

Computer Science

4

Nitrogen Lines: Data Bases, Nitrogen Lines: Solar Atmosphere, Molecular Lines: Nitrogen Lines, Molecular Lines: Tests

Scientific paper

For NH bands region near λ 336 nm the data from Kurucz database (1993): the list of atomic lines LOWLINES.DAT from CD-ROM N 1 and the molecular line lists from CD-ROM N 18 are tested and corrected using the spectrum of the Sun as a star. The nitrogen abundances indicators are selected for spectral resolution of 0.0025 nm and 0.02 nm. The effect of a line list completeness on the nitrogen abundance estiamtes is considered.

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