Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..760m&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 93, March 1987, p. 760-767. Research supported by the Applied Research Corp.
Astronomy and Astrophysics
Astronomy
5
Astrometry, Cepheid Variables, Distance Measuring Equipment, Double Stars, Interferometry, Spaceborne Astronomy, B Stars, Magellanic Clouds, Point Sources, Separation, Stellar Mass, Supergiant Stars
Scientific paper
It is demonstrated that an idealized version of an instrument specifically designed to resolve double stars with different colors can increase the resolving power of a conventional interferometer by more than a factor of 30, and may enable a 5 m baseline interferometer to provide useful measurements of point sources separated by only a few times 10 to the -5th arcsec. An obvious application for such a device is to measure the angular separations of double-lined spectroscopic binary Cepheids. In combination with radial velocities, the angle measurements provided by a spaceborne interferometer with a baseline of only 5 m can determine the distances to approximately 40 Milky Way Cepheids from Newton's laws and Euclidean geometry. This number should be adequate to calibrate the period-luminosity relationship directly - which amounts to bypassing two rungs of the cosmic distance ladder. The instrument may also be able to resolve about 25 M supergiant +B star systems in the LMC - thereby placing the large cloud on a fundamental distance scale.
Endal Andrew S.
Massa Derck
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