Comptel^(26)Al1.8 MeV 与SNR和 W-R 星相关分析

THE CORRELATION ANALYSIS ON COMPTEL (26)~Al WITH SNR AND W-R STARS

利用Comptel的观测处理结果，对SNR及W－R星与1．8MeVγ射线沿银经的分布做了拟合优度的检验和相关分析．K—S统计检验的结果认为，在α＝0．10水平上W—R星与1．8MeV来自同样的分布．相关分析的结果也表明W—R星与1．8MeV的分布有较好的相关性．

The current viewpoint of the possible sources of 26Al is the massive stars, the Wolf-Rayet stars, the AGB stars, the supernovae of Type Ⅱ and Ⅰb and novae. Taking advantage of the data processing results of the Comptel observations, the correlation of the 1.8 MeV γ-ray with the SNR and the W-R stars is analyzed. The goodness-of-fit of their distributions along the galactic longitude is studied. According to the results of K-S tests, the W-R stars and 1.8MeV come from the same distribution (α=0.10). The correlation analysis also shows that the W-R stars is correlative fairly to the 1.8 MeV.