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SUMMARY: The dark matter distribution in galaxies and clusters with new  d
 ynamical mass modeling methods - Gary Mamon\, IAP\, France
DTSTART:20081120T163000Z
DTEND:20081120T173000Z
UID:TALK13620@talks.cam.ac.uk
CONTACT:Dr. Vasily Belokurov
DESCRIPTION:Abstract not available
LOCATION:Sackler Lecture Theatre\, IoA (tea at 4.00 pm)
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