摘要
依据观测获得的5颗晚型星:λAnd,κCet,61CygA,αCas和βCet的高分辨率、高信噪比的光谱,采用谱线塞曼致宽的谱线轮廓叠加法和利用大量FeI的多重线统计分析方法,成功地测定了这些星的磁场和磁场覆盖因子。
e have obtained highresolution (R=4×10~4), high signaltonoise ratio (S/N =200~300) CCD spectra of λ And,κ Cet and 61 Cyg A using the 2.16 m telescope with echelle spectrograph of Beijing Astronomical Observatory in 1995.CCD spectra of α Cas and β Cet with high resolution (R=6×10~4), and high signaltonoise ratio (S/N=300~400) were obtained using the Coud′e spectrograph of Yunnan Observatory in 1994. In this paper, the preliminary results of magnetic field determinations for five latetype stars are presented. We use two methods,i.e. the profileaddition technique of spectral profiles of Zeeman broadening and StenfloLindegren statistical analysis.
基金
国家自然科学基金