Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mnras.356.1256c&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 356, Issue 4, pp. 1256-1262.
Astronomy and Astrophysics
Astronomy
Stars: Abundances, Stars: Chemically Peculiar, Stars: Individual: Hr 8216
Scientific paper
An elemental abundance analysis of the cool magnetic CP star HR 8216 (= HD204411) was performed using 2.4 Åmm-1 Dominion Astrophysical Observatory Reticon exposures covering λλ3830-4770 with a typical signal-to-noise ratio of 200 taken with the long camera of the 1.22-m telescope. The spectrograms were measured interactively with the graphics computer program REDUCE. The fine analysis used an ATLAS9 metal-rich model atmosphere, the predictions of which best-matched the optical region fluxes and the Hγ profile. The anomalies of HR 8216 are primarily an enhancement of many iron peak elements with the rare earths elements much less enhanced than in many similar cool magnetic CP stars. Using the results of the fine analysis the spectrum was synthesized. Comparison with the observed spectrum showed that the agreement is good but did not fully account for all of the observed line spectrum.
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