Translator Disclaimer
Paper
5 July 2000 How AMBER will contribute to the search for brown dwarfs and extrasolar giant planets
Author Affiliations +
Abstract
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.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Damien Segransan, Jean-Luc Beuzit, Xavier Delfosse, Thierry Forveille, Michel Mayor, Christian Perrier-Bellet, and F. Allard "How AMBER will contribute to the search for brown dwarfs and extrasolar giant planets", Proc. SPIE 4006, Interferometry in Optical Astronomy, (5 July 2000); https://doi.org/10.1117/12.390218
PROCEEDINGS
8 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT


Back to Top