High angular resolution stellar interferometry

Details High angular resolution stellar interferometry High angular resolution stellar interferometry

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976pasau...3...26d&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 10th, Sydney, Australia, May 12-14, 1976.) Astronomical Society of A

Astronomy and Astrophysics

Astronomy

8

Angular Resolution, Astronomical Photometry, Interferometry, Binary Stars, Cepheid Variables, Diameters, High Resolution, Hot Stars, Michelson Interferometers, Size Determination, Stellar Atmospheres

Scientific paper

After a brief discussion of the historical development of stellar interferometry, the astronomical potential of high angular resolution stellar interferometry is considered. Attention is given to interferometric measurements of emergent fluxes and effective temperatures for single stars, stellar radii, binary stars, and Cepheid variables. Attention is also given to the design of different types of high angular resolution stellar interferometers including the intensity interferometer and three kinds of amplitude interferometers: the Michelson, heterodyne, and speckle interferometers.

Affiliated with

Also associated with

No associations

Rating

High angular resolution stellar interferometry does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with High angular resolution stellar interferometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High angular resolution stellar interferometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1416325