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SUMMARY:Mass function of the stellar remnants in the Milky Way - Lukasz Wy
 rzykowski (Warsaw)
DTSTART:20150708T121500Z
DTEND:20150708T124500Z
UID:TALK59961@talks.cam.ac.uk
CONTACT:28811
DESCRIPTION:Gravitational microlensing is the only technique allowing for 
 detecting\nindividual and non-interacting stellar remnants\, in particular
  neutron stars\nand black holes. I will present candidates for stellar rem
 nant microlenses\nfound in the decade-long photometric monitoring of hundr
 ed million stars\ntowards the Galactic Bulge by the Polish OGLE project. I
  will show how\ncombining photometry from OGLE and astrometry from Gaia mi
 ssion will\nultimately solve the uncertainties in the mass measurements of
  stellar\nremnants.\n
LOCATION:Sackler Lecture Theatre\, IoA
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