Observations of binary stars by speckle interferometry. I

Details Observations of binary stars by speckle interferometry. I Observations of binary stars by speckle interferometry. I

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.183..701m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 183, June 1978, p. 701-710. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

32

Binary Stars, Diffraction Patterns, Interferometry, Speckle Patterns, Stellar Spectrophotometry, Variable Stars, Astronomical Spectroscopy, Cepheid Variables, Radial Velocity

Scientific paper

Speckle interferometry has been used to study a large number of binary-star systems and variable stars. Thirty-five observations on 30 objects are presented. These objects include six radial-velocity or photometric variable stars. Of these, new components are reported for the systems Epsilon UMa, Gamma Boo, and W Sgr; the system Sigma Sco is resolved into three components, confirming the results of Nather, Churms, and Wild (1974). The technique provides a very accurate means of measuring the separations of these systems.

Affiliated with

Also associated with

No associations

Rating

Observations of binary stars by speckle interferometry. I 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 Observations of binary stars by speckle interferometry. I, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of binary stars by speckle interferometry. I will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-791076