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Tidal disruption of asteroids by supermassive black holes

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The compact radio source Sgr A* at the centre of our Galaxy harbours a super-massive black hole. and is therefore the nearest laboratory for testing the super-massive black hole astrophysics and environment. Since it is not an active galactic nucleus. it also offers the possibility of observing the capture of low-mass objects. https://www.roneverhart.com/Brach-s-Natural-Sources-Candy-Corn-10-Ounce-Bag/
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