Towards a Three-Dimensional Model of the Galaxy
نویسندگان
چکیده
We present preliminary results of our modelling of the J,K,L and M band emission detected by the DIRBE instrument on the COBE satellite. Our model includes the contribution of Zodiacal light and a three-dimensional model for the distribution of dust based upon DIRBE observations of dust emission at 240 microns. Our approach enables us to construct dust removed maps of our Galaxy that we will use to model the structure of the bar, the spiral structure of Galaxy and the shape of the disk.
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تاریخ انتشار 2007