2010 Fiscal Year Final Research Report
Formation Mechanism for Supermassive Black Holes through Multi-dimensional radiationMmagnetohydrodynamic Simulations
Project/Area Number |
20740115
|
Research Category |
Grant-in-Aid for Young Scientists (B)
|
Allocation Type | Single-year Grants |
Research Field |
Astronomy
|
Research Institution | National Astronomical Observatory of Japan |
Principal Investigator |
OHSUGA Ken National Astronomical Observatory of Japan, 理論研究部, 助教 (90386508)
|
Project Period (FY) |
2008 – 2010
|
Keywords | ブラックホール / ガス円盤 / ジェット / 数値計算 |
Research Abstract |
We performed the global 2D-radiation magnetohydrodynamic simulations of the accretion disks and jets around black holes. Three distinct accretion disks are for the first time reproduced by one numerical code. Especially, we found a new type jet : radiatively-driven, magnetically-collimated jet.
|