Twenty-eight angular diameters for late-type stars by the lunar occultation technique

Details Twenty-eight angular diameters for late-type stars by the lunar occultation technique Twenty-eight angular diameters for late-type stars by the lunar occultation technique

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..247r&link_type=abstract

Astronomical Journal, vol. 84, Feb. 1979, p. 247-256.

Astronomy and Astrophysics

Astronomy

43

Astronomical Photometry, Astronomy, Diameters, Infrared Astronomy, Late Stars, Lunar Occultation, Variable Stars, Computerized Simulation, Diffraction Patterns, Dimensional Measurement, Error Analysis, Graphs (Charts), Mira Variables, Radio Telescopes, Scintillation, Signal To Noise Ratios

Scientific paper

New angular diameter measurements obtained with an infrared photometer are reported. The stars observed include three Mira variables and nine cool IRC objects. Repeat measurements are reported for five stars. The observations include numerous daytime and reappearance events. Several results obtained with the 4-m telescope verify the value of a large aperture for the measurement of angular diameters as small as 1.5-2.5 milliarcsec.

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