A search for companions to nearby brown dwarfs:: The binary DENIS-PJ1228.2-1547

Hubble Space Telescope imaging observations of two nearby brown dwarfs, DENIS-P J1228.2-1547 and Kelu 1, made with the near-infrared camera and multiobject spectrometer (NICMOS), show that the DENIS object is resolved into two components of nearly equal brightness with a projected separation of 0.275 are second (5 astronomical units for a distance of 18 parsecs), This binary system will be able to provide the first dynamical measurement of the masses of two brown dwarfs in only a few years. Upper Limits to the mass of any unseen companion in Kelu 1 yield a planer of 7 Jupiter masses aged 0.5 x 10(9) years, which would have been detected at a separation Larger than about 4 astronomical units. This example demonstrates that giant planets could be detected by direct imaging if they exist in Jupiter-like orbits around nearby young brown dwarfs.