Creating AKARI Far-Infrared Diffuse Emission Maps in the All Sky Survey and a Study of the Formation Processes of Molecular Clouds

我们已经完成了处理AKARI远红外数据的管道程序，并刚刚开始制作AKARI全天图像。AKARI团队成员现在可以获得AKARI朝向人马座银河系中心区域的图像。此外，我们还完成了敏感的变色龙暗星云AKARI图像的定标。对图像的统计分析使我们得出这样的结论：星云中的湍流在确定那里新形成的星星的质量方面起着关键作用。

We have completed the pipeline programs to process the AKARI far-infrared data, and have just started making AKARI All-Sky images. The AKARI images toward the Galactic center region in Sagittarius are now available to AKARI team members. In addition, we have finished calibrating the sensitive AKARI images of the Chamaeleon dark nebula. The statistical analysis of the images leads us to the conclusion that the turbulence in the nebula plays a key role in determining the mass of a star newly forming there.