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

Bibcode
2000SPIE.4006..269S
Segransan, Damien; Beuzit, Jean-Luc; Delfosse, Xavier; Forveille, Thierry; Mayor, Michel; Perrier-Bellet, Christian; Allard, F.
Referencia bibliográfica

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

Fecha de publicación:
7
2000
Número de autores
7
Número de autores del IAC
1
Número de citas
11
Número de citas referidas
7
Descripción
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.
Tipo
Sin árbitro

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