Abundance and F values needed to interpret adequately the high resolution IUE spectra

Details Abundance and F values needed to interpret adequately the high resolution IUE spectra Abundance and F values needed to interpret adequately the high resolution IUE spectra

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281a.377f&link_type=abstract

In ESA, A Decade of UV Astronomy with the IUE Satellite, Volume 1 p 377-379 (SEE N89-10682 01-89)

Astronomy and Astrophysics

Astronomy

Abundance, Iue, Spaceborne Astronomy, Stellar Atmospheres, Ultraviolet Astronomy, Ultraviolet Spectra, High Resolution, Spectral Resolution

Scientific paper

To establish the real needs to interpret correctly a high resolution IUE spectrum, a rough estimate of what would be the abundance or the f minimal values that correspond to isolated lines in the limit of detection given by instrumental resolution is made. The need to develop the determination or calculation of atomic data concerning very weak spectral lines is stressed. Thus, with more complete and reliable atomic data, systematic synthetic spectra calculations could lead to better understanding of physical conditions of stellar atmospheres.

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