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Spectrophotometry of speckle binary stars. III

Al-Wardat, M. A.

Spectrophotometric observations of a third set consisting of 11 stars of speckle interferometric binaries are presented. Observations covered the range 3700-8400 Å with a resolution of 18 Å. Results are presented in the form of the measured flux corrected for atmospheric extinction in the units of erg/cm²·s·sÅ, with no corrections for i…

Reduction of the binary stars Δm measurements, obtained with the speckle interferometer of BTA of SAO RAS, into the standard photometric system

Zhuchkov, R. Ya.

For magnitude difference, measured with the speckle interferometer of the 6m telescope of SAO RAS, corrections for transformation from interferometer's photometric system into standard Johnson-Cousins V R I bands are calculated. The reduction accuracy is 0.01^m - 0.02^m. To determine the correction one has to know the magnitude…

Spectrophotometry of speckle binary stars III

Al-Wardat, M. A.

Spectrophotometric observations of a third set consisting of 11 stars of speckle interferometric binaries are presented. Observations covered the range 3700-8400 Å, with a resolution of 18 Å. Results are presented in the form of the measured flux corrected for atmospheric extinction in the units of erg/cm²\cdot s \cdot Å, with no correc…