Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 173
... tion . The midinfrared camera built by Arens et al . ( 1990 ) for the Keck Telescope utilizes a separate Motorola DSP56001 on each of the twenty readout lines coming from a 20 × 64 infrared array . NASA's Infrared Telescope Facility ...
... tion . The midinfrared camera built by Arens et al . ( 1990 ) for the Keck Telescope utilizes a separate Motorola DSP56001 on each of the twenty readout lines coming from a 20 × 64 infrared array . NASA's Infrared Telescope Facility ...
Page 188
" • Procedures for Radial Velocities of Close Binaries from Spectra Obtained. tion to the use of the very low - noise detectors and highthroughput optics . 6. SUMMARY We have calculated the wavefront reconstruction errors for Shack ...
" • Procedures for Radial Velocities of Close Binaries from Spectra Obtained. tion to the use of the very low - noise detectors and highthroughput optics . 6. SUMMARY We have calculated the wavefront reconstruction errors for Shack ...
Page 225
... tion ) . K = 12.5kЄM1.0 ( 10 ) ( 11 ) -0.7 wd as an approximate mass - radius relaThis reproduces the slope of the empirical relation . For a typical white dwarf M1≈0.7 , so the intercept is correct when ke = 0.007 . Now k cannot ...
... tion ) . K = 12.5kЄM1.0 ( 10 ) ( 11 ) -0.7 wd as an approximate mass - radius relaThis reproduces the slope of the empirical relation . For a typical white dwarf M1≈0.7 , so the intercept is correct when ke = 0.007 . Now k cannot ...
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