TY - JOUR
T1 - Recent science results with the two-telescope IOTA
AU - Millan-Gabet, Rafael
AU - Pedretti, Ettore
AU - Monnier, John D.
AU - Traub, Wesley A.
AU - Schloerb, F. Peter
AU - Carleton, Nathaniel P.
AU - Ragland, Sam
AU - Lacasse, Marc G.
AU - Danchi, William C.
AU - Tuthill, Peter G.
AU - Perrin, Guy S.
AU - Coudé du Foresto, Vincent
PY - 2003/2/1
Y1 - 2003/2/1
N2 - The IOTA (Infrared Optical Telescope Array) has been routinely operating
with two-telescopes since 1994, a mode destined to become obsolete
following its recent conversion to a three-telescope array. In
two-telescope mode, the IOTA has made numerous scientific and technical
contributions, see e.g. our list of publications at
http://cfa-www.harvard.edu/cfa/oir/IOTA/PUBLI/publications.html. We
present preliminary results on three different topics using recent data
from the two-telescope IOTA: (1) measurements of Mira star diameters
simultaneously in three different near-infrared spectral bands, (2)
measurement of the characteristic size and shape of the source of
near-infared emission in the x-ray binary system CI Cam, and (3)
aperture synthesis of the Carbon star V Hydrae combining data from the
IOTA and from aperture masking at the Keck-I telescope.
AB - The IOTA (Infrared Optical Telescope Array) has been routinely operating
with two-telescopes since 1994, a mode destined to become obsolete
following its recent conversion to a three-telescope array. In
two-telescope mode, the IOTA has made numerous scientific and technical
contributions, see e.g. our list of publications at
http://cfa-www.harvard.edu/cfa/oir/IOTA/PUBLI/publications.html. We
present preliminary results on three different topics using recent data
from the two-telescope IOTA: (1) measurements of Mira star diameters
simultaneously in three different near-infrared spectral bands, (2)
measurement of the characteristic size and shape of the source of
near-infared emission in the x-ray binary system CI Cam, and (3)
aperture synthesis of the Carbon star V Hydrae combining data from the
IOTA and from aperture masking at the Keck-I telescope.
M3 - Article
VL - 4838
SP - 202
EP - 209
JO - Interferometry for Optical Astronomy II
JF - Interferometry for Optical Astronomy II
ER -