A search for companions to nearby brown dwarfs: the binary DENIS-P J1228.2-1547 |
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Authors: | Martin Brandner Basri |
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Affiliation: | Department of Astronomy, University of California, Berkeley, CA 94720, USA. Jet Propulsion Laboratory/Infrared Processing and Analysis Center, Mail Code 100-22, Pasadena, CA 91125, USA. |
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Abstract: | 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 arc 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 planet 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. |
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