The DWARF Project Eclipsing Binaries:Precise Clocks to Detect Extrasolar Planets(i) systems with K or/and M dwarf components(ii) systems with hot subdwarf(sd) a
OUTLINE Background NG-DRAPS Future Plan New technology→Data Rate VLBI High stability frequency standard High accuracy time synchronization High speed recording
Outline Background of LSI+61 303 VLBA Observations Results Future Plan Background of LSI+61 303Binary:Be star(B0)+compact object Microquasar or Pulsar wind D~2 k