BLACK HOLE at the GALACTIC CENTER

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Presentation transcript:

BLACK HOLE at the GALACTIC CENTER Paul T.P. Ho Academia Sinica IAA GSMT 04.28.2003

Center of the Galaxy Sgr A* GSMT 04.28.2003

WHY the GALACTIC CENTER? Nearest Supermassive Black Hole Inflow and Accretion Rate Connection to the Galactic Disk Best Resolution and Sensitivity Paradigm for AGN’s GSMT 04.28.2003

Orbital Motions Around SgrA. Schödel et al. Nature 419,694 (10. 17 VLT 8-m UT4: NAOS/CONICA Diffraction Limited : 56mas @ 2.18m AOS closed on supergiant IRS7 (6" N): Strehl ratio over 40% Seeing Halos removed by Wiener Filter GSMT 04.28.2003

2.18m Images of Galactic Center GSMT 04.28.2003

Galactic Center Proper Motions GSMT 04.28.2003

Orbit of S2 Around SgrA* GSMT 04.28.2003

Orbit of S2 Around SgrA* Semimajor Axis: 0.119" = 5.5 lightdays Orbital Period: 15.2 years Pericentre Distance: 15mas = 17 lighthours = 124 AU = 2100 Rsch = 70 Rtidal Binding Mass: 3.7 x 106 Mo GSMT 04.28.2003

Recap the Proper Motions GSMT 04.28.2003

How Much Better ? Increased Resolution and Sensitivity. Detect and Track Fainter Stars. Detect even Faster Motions? Better Constraints on Orbits, Accelerations. Detect Tidal Distortions? Detect Relativistic Motions at 100 Rsch ? GSMT 04.28.2003