The photometric orbital elements of the eclipsing variable, RZ Pyxidis, are derived by means of Fourier series from photoelectric observations which were made by Michel Breger (1964). Physical dimensions and a model of the system are suggested here.
목차
Abstract Ⅰ. 緖論 Ⅱ. 理論的 考察 Ⅲ. Data 分析 및 軌道要素計算 Ⅳ. 結論 謝辭 References