| Project/Area Number |
24K17100
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| Research Category |
Grant-in-Aid for Early-Career Scientists
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| Allocation Type | Multi-year Fund |
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| Review Section |
Basic Section 16010:Astronomy-related
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| Research Institution | National Astronomical Observatory of Japan |
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Principal Investigator |
Saha Piyali 国立天文台, アルマプロジェクト, 特任研究員 (40991055)
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| Project Period (FY) |
2024-04-01 – 2026-03-31
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| Project Status |
Granted (Fiscal Year 2024)
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| Budget Amount *help |
¥4,030,000 (Direct Cost: ¥3,100,000、Indirect Cost: ¥930,000)
Fiscal Year 2025: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
Fiscal Year 2024: ¥2,340,000 (Direct Cost: ¥1,800,000、Indirect Cost: ¥540,000)
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| Keywords | Magnetic fields / High-mass star formation / Polarization / Massive stars / Dust continuum emission |
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| Outline of Research at the Start |
The scarcity of information about the dynamical stages of the HMPSCs necessitates the study of energy balance between turbulence, gravity, and B-field. We will study six HMPSCs to understand the role of B-field in their formation. Adding gravity and turbulence, we will study their dynamical stages.
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