Abundance determination for the sharp-lined A2V star HD72660 using high resolution ultraviolet spectra

Details Abundance determination for the sharp-lined A2V star HD72660 using high resolution ultraviolet spectra Abundance determination for the sharp-lined A2V star HD72660 using high resolution ultraviolet spectra

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..519d&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

We determined the abundance of several elements for the A2V star HD72660 using ultraviolet spectra from IUE archives and an archival ELODIE echelle spectrum. The simultaneous usage of optical and UV spectra allows to synthesize a large number of lines of several chemical elements. Synthesis is more reliable in the optical range where the line density is less.

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