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Galactic Center Rotation Curve and Mass Yoshiaki Sofue (Meisei Uni
Galactic Center Rotation Curve and Mass Yoshiaki Sofue (Meisei Uni.) Nagoya University
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1. Log Rotation Curve 2. Mass models 3. Galactic Center RC 4
1. Log Rotation Curve 2. Mass models 3. Galactic Center RC 4. BH - Bulge – Disk -DH
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1. Rotation Curve
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銀河中心
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inside/outside Solar Circle
Rotation velocities inside/outside Solar Circle
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Solar Circular Velocity V0=200 km/s @ R0=8kpc
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2. Mass Model
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RC Fitting by (1) Bulge: de Vaucouleurs Law (2) Disk: Exponential
(3) Dark Halo: NFW
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de V ∝ exp(-r1/4) Expo. Plummer Kepler
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(1) Bulge de Vaucouleurs: exp(-r1/4)
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(2) Disk: Exponential
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(3) Dark Halo NFW Density Profile
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Sofue, Honma, Omodaka 2009
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Volume Densities for Bulge, Disk, and Halo(Isoth, NFW, Burkert)
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Total Masses Dark Halo Expo. Disk de Vaucl. Bulge
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3. Grand Rotation Curve
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Solar Circular Velocity V0=200 km/s @ R0=8kpc
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Define: Vrot =Vvirial≒ √2 VGC
Rotation curve at R>30 kpc assuming random motion of satellite galaxies Define: Vrot =Vvirial≒ √2 VGC
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MW ⇔ M31 border de V. Bulge Milky Way GRC Expo. Disk NFW Halo
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4. Galactic Center & BH
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質量空白域 or DM cusp Rc
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銀河質量研究の空白領域 BH - Bulge Log R
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BH formation in core/cusp
Rc
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BH – Bulge – Disk NGC 3079
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GC CO map & LV diagrams
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CO LV diagrams
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Terminal Velocities
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GC Rotation Curve
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Galaxy Rotation Curve
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Surface Mass Density
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Deconvolution of RC
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Vaucouleurs vs Exponential
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Density (Semi Log)
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Density (Log Log)
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質量分布ー直接導出 > >
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SMD : Obs vs Model
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Comparison with Genzel et al. 94
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RC Fitting Result: BH Bulge 1 : Exp. Sphere (3) Bulge 2: Exp. Sphere
(4) Exp. Flat Disk (5) NFW Dark Halo
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PASJ submitted 2013
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Further Analysis of Activity in known Gravity Environment
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