Inner radii of dust shells and stellar diameters obtained by an infrared stellar interferometer at 11 micron wavelength
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D. Hale | C. Townes | M. Bester | W. Danchi | N. Geis | L. Greenhill | C. Degiacomi | B. Lopez
[1] William C. Danchi,et al. Analysis of visibility data from the University of California/Berkeley Infrared Spatial Interferometer: radiative transfer modeling and results on fifteen stars , 1994, Astronomical Telescopes and Instrumentation.
[2] William C. Danchi,et al. University of California/Berkeley Infrared Spatial Interferometer: recent system upgrades and analysis of atmospheric fluctuations , 1994, Astronomical Telescopes and Instrumentation.
[3] C. Townes,et al. Characteristics of dust shells around 13 late-type stars. , 1994 .
[4] M. Bester,et al. Analysis of Visibility Data from the U.C. Berkeley Infrared Spatial Interferometer-Radiative Transfer Modeling and Results on Fifteen Stars. , 1994 .
[5] William C. Danchi,et al. Distribution of dust about ο Ceti and α Orionis based on 11 micron spatial interferometry , 1991 .
[6] William C. Danchi,et al. Location and Phase of Dust Formation in IRC +10216 Indicated by 11 Micron Spatial Interferometry , 1990 .