| Project/Area Number |
19740094
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Astronomy
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| Research Institution | The University of Tokyo (2008-2009)
Hokkaido University (2007) |
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Principal Investigator |
NOZAWA Takaya The University of Tokyo, 数物連携宇宙研究機構, 特任研究員 (90435975)
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| Research Collaborator |
KOZASA Takashi 北海道大学, 大学院・理学研究院, 教授 (90263368)
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| Project Period (FY) |
2007 – 2009
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| Project Status |
Completed (Fiscal Year 2009)
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| Budget Amount *help |
¥3,770,000 (Direct Cost: ¥3,200,000、Indirect Cost: ¥570,000)
Fiscal Year 2009: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2008: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
Fiscal Year 2007: ¥1,300,000 (Direct Cost: ¥1,300,000)
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| Keywords | ダスト(星間塵) / 超新星爆発 / 超新星残骸 / 可視光赤外線観測 / 物質進化 / 星間衝撃波 / 質量放出 / ダスト / 衝撃波 / 第一世代星 / 超金属欠乏星 / 星間減光曲線 / 赤外線 |
|---|
| Research Abstract |
We investigated the formation of dust in the ejecta of supernovae that are considered to be sources of interstellar dust in the early universe. Then we studied the evolution of the newly formed dust in the shocked gas within the supernova remnants and revealed the size distribution and mass of the dust injected into the interstellar medium. Based on the results of these calculations, we estimated UV-optical extinction curves expected in the early universe. We also demonstrated how the formation process of dust depends on the type of supernovae through the varying thickness of their outer envelopes.
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