How AMBER will contribute to the search for brown dwarfs and extrasolar giant planets

Details How AMBER will contribute to the search for brown dwarfs and extrasolar giant planets How AMBER will contribute to the search for brown dwarfs and extrasolar giant planets

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4006..269s&link_type=abstract

Proc. SPIE Vol. 4006, p. 269-276, Interferometry in Optical Astronomy, Pierre J. Lena; Andreas Quirrenbach; Eds.

Astronomy and Astrophysics

Astronomy

6

Scientific paper

Various radial velocity surveys have now produced a number of candidates Very Low Mass Stars, Brown Dwarfs and Giant Extrasolar Planets to nearby G, K and M dwarfs. Building upon our experience in High Angular Resolution imaging, radial velocities measurements and atmosphere modeling, we discuss the detectability of Brown Dwarfs and Extrasolar Giant Planets with AMBER--the near-infrared instrument of the VLTI--using differential interferometry in low spectral dispersion mode.

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