Bulletin of the Korean Space Science Society (한국우주과학회:학술대회논문집(한국우주과학회보))

The Korean Space Science Society (한국우주과학회)
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A Spectroscopic Abundance Study of Dwarf Cepheid V1719 Cygni

  • Kim, Chulhee- (Department of Earth Science Education Chonbuk National University, KOREA) ;
  • Kozo-Sadakane (Astronomical Institute Osaka Kyoiku University, JAPAN)
  • Published : 1992.10.01
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Abstract

Spectroscopic CCD observations were carried out for V 1119 Cygni and the spectrum inthe visual region is analysed relative to the SLln with a line-blanketed convective modelatmosphere. Adopted atmospheric parameters are : an effective temperature ( Teff) =7000 K, a surface gravity log g = 3.4. Although our result is dependent onmicroturbulent velocity and damping constant, it was found that Mg in V1719 Cygni isnearly solar, or underabundant by 0.2 to 0.3 dex according to the analysis of5172.684A Mg I line which is relatively free from blending. This is inconsistentwith the previous photometric result wh(:re V1719 Cygni was known as anabnormally metal rich variable.

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