Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared

@inproceedings{Woodruff2004InterferometricOO,
  title={Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared},
  author={H. Woodruff and Maren Eberhardt and Thomas Driebe and K. H. Hofmann and Keiichi Ohnaka and A Richichi and Dieter Schertl and Markus Schoeller and Miklas Scholz and Gerd Weigelt and Markus Wittkowski and P. R. Wood Max Planck Institute for Radioastronomy and Bonn and European Southern Observatory and Institute of Theoretical Astrophysics and University of Heidelberg and Institute of Radio Astronomy and School of Cosmic Physics and University of Western Sydney and Research School of Astronomy and Astrophysics and Australian Nat. Univ. and Weston Creek},
  booktitle={SPIE Astronomical Telescopes + Instrumentation},
  year={2004}
}
We present K-band commissioning observations of the Mira star prototype o Cet obtained at the ESO Very Large Telescope Interferometer (VLTI) with the VINCI instrument and two siderostats. The observations were carried out between 2001 October and December, in 2002 January and December, and in 2003 January. Rosseland angular radii are derived from the measured visibilities by fitting theoretical visibility functions obtained from center-to-limb intensity variations (CLVs) of Mira star models… 
Tests of stellar model atmospheres by optical interferometry. IV. VINCI interferometry and UVES spec
Aims. We present coordinated near-infrared K-band interferometric and optical spectroscopic observations of the M 1.5 giant α Cet (Menkar) obtained with the instruments VINCI and UVES at the Paranal
Mid-infrared interferometry of the Mira variable RR Sco with the VLTI MIDI instrument
We present the results of the first mid-infrared interferometric observations of the Mira variable RR Sco with the MID-infrared Interferometer (MIDI) coupled to the European Southern Observatory's
Joint VLBA/VLTI Observations of the Mira Variable S Orionis
We present the first coordinated Very Long Baseline Array (VLBA) / Very Large Telescope Interferometer (VLTI) measurements of the stellar diameter and circumstellar atmosphere of a Mira variable
Tests of stellar model atmospheres by optical interferometry III: NPOI and VINCI interferometry of
Aims: We present a comparison of the visual and NIR intensity profile of the M0 giant gamma Sagittae to plane-parallel ATLAS 9 as well as to plane-parallel & spherical PHOENIX model atmospheres.
The K-band intensity profile of R Leonis probed by VLTI/VINCI ⋆
We present near-infrared K-band interferometric measurements of the Mira star R Leonis obtained in April 2001 and January 2002 withVLTI/VINCI. The April 2001 measurements indicate a center-to-limb
The keck aperture masking experiment: Multiwavelength observations of six Mira variables
The angular diameters of six oxygen-rich Mira-type long-period variables have been measured at various NIR wavelengths using the aperture-masking technique in an extensive observing program from 1997
THE KECK APERTURE MASKING EXPERIMENT: SPECTRO-INTERFEROMETRY OF THREE MIRA VARIABLES FROM 1.1 TO 3.8 μm
We present results from a spectro-interferometric study of the Miras o Cet, R Leo, and W Hya obtained with the Keck Aperture Masking Experiment from 1998 September to 2002 July. The spectrally
J, H, K spectro-interferometry of the Mira variable S Orionis
Aims. We present J, H, K spectrally dispersed interferometry with a spectral resolution of 35 for the Mira variable S Orionis. We aim at measuring the diameter variation as a function of wavelength
New Measurements of the Radio Photosphere of Mira Based on Data from the JVLA and ALMA
We present new measurements of the millimeter wavelength continuum emission from the long period variable Mira (oCeti) at frequencies of 46, 96, and 229 GHz ( 7 l » , 3, and 1 mm) based on
The Mira variable S Orionis: relationships between the photosphere, molecular layer, dust shell, and SiO maser shell at 4 epochs
Aims. We present the first multi-epoch study that includes concurrent mid-infrared and radio interferometry of an oxygen-rich Mira star. Methods. We obtained mid-infrared interferometry of S Ori with