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MPIfR
Optical & Infrared
Interferometry Group
Weigelt, G., Balega, Y., Hofmann, K.-H., Scholz, M.
First diffraction-limited speckle masking observations of the Mira variable R Cas with the 6m SAO telescope
Astronomy and Astrophysics 316, L21-L24 (1996)
We present the first diffraction-limited speckle masking observations of a Mira star with the Russian 6m SAO telescope. At 700 and 714nm wavelength a resolution of 30 milli-arcsec was achieved. The reconstructed true images are the images with the highest resolution obtained up to now in this wavelength region. The speckle interferograms of R Cas were recorded through interference filters with center wavelength/ bandwidth of 714nm/6nm (strong TiO band absorption) and 700nm/6nm (moderate TiO absorption). The two reconstructed images show that the azimuthally averaged 700 and 714nm uniform-disk diameters of R Cas are 36mas +/- 2mas and 49mas +/- 2mas, respectively. In the 700nm and 714nm images the disks of R Cas are non-uniform and elongated along position angle 52 +/- 7 degrees and 57 +/- 7 degrees, respectively. The size (elliptical uniform disk fit) of the elongated disks is about 33.3mas x 38.7mas (axial ratio 0.86) in the 700nm pseudo-continuum filter and 42.3mas x 55.6mas (axial ratio 0.76) in the 714nm TiO absorption band filter. We discuss briefly theoretical aspects of these and previous observations.
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