| Budget Amount *help |
¥8,450,000 (Direct Cost: ¥6,500,000、Indirect Cost: ¥1,950,000)
Fiscal Year 2020: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
Fiscal Year 2019: ¥2,080,000 (Direct Cost: ¥1,600,000、Indirect Cost: ¥480,000)
Fiscal Year 2018: ¥2,340,000 (Direct Cost: ¥1,800,000、Indirect Cost: ¥540,000)
Fiscal Year 2017: ¥2,210,000 (Direct Cost: ¥1,700,000、Indirect Cost: ¥510,000)
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| Outline of Final Research Achievements |
We have quantified the interstellar medium (ISM) and coscmi-rays (CRs) based on GeV gamma-ray and multiwavelength obervations, as well as studied the CR accelerator data in detail. On the latter we have published a detailed study of the X-ray morphology of VER J2019+368. On the former, we published the analysis of Chamaeleon molecular clouds (in particular the study of non-linearity between the dust emission and ISM density) and high-latitude HI clouds (in particular measurement of ISM density without an assuption of spin temperature). In addition, we have shown that by using HI line profile we can significantly improve the accuracy of ISM/CR measurements. The method has been applied to the MBM 53-55 molecular clouds and Pegasus loop region, and a dedicated paper is in preparation.
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