Abstract
Ten years after Paczyński's proposal to use gravitational microlensing as a tool for discovering dark stars and four years after the identification of the first candidate events, searches for microlensing events have opened a new window in astronomy and started to yield quantitative information on the contribution of dark compact objects to the dark halo of the Galaxy. A review of the results obtained so far is presented, along with recent highlights in the direction of the Small Magellanic Cloud.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
