Angular diameter measurements of Alpha Orionis, VY Canis Majoris, and IRC + 10216 at 8.3, 10.2, and 11.1 micrometers

Details Angular diameter measurements of Alpha Orionis, VY Canis Majoris, and IRC + 10216 at 8.3, 10.2, and 11.1 micrometers Angular diameter measurements of Alpha Orionis, VY Canis Majoris, and IRC + 10216 at 8.3, 10.2, and 11.1 micrometers

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...214l..85m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 214, June 1, 1977, p. L85-L89. NSF-supported research.

Astronomy and Astrophysics

Astronomy

51

Infrared Astronomy, Size Determination, Stellar Envelopes, Carbon Stars, Data Reduction, Interstellar Masers, M Stars

Scientific paper

Nine stars have been observed interferometrically at 8.3, 10.2, and 11.
1 microns using an east-west baseline of 2.0 m. Three stars, Alpha Ori,
VY CMa, and IRC + 10216, and the Jovian satellite Callisto, were
resolved at one or more wavelengths. Betelgeuse was also observed with a
3.0-m baseline.

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