Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 186
... Figure 4 shows the number of maximum correctable terms Nmax for a given number of subapertures Nspot This figure is drawn by plotting the Nat value which gives the minimum residual wavefront error E for a given & value . Using this ...
... Figure 4 shows the number of maximum correctable terms Nmax for a given number of subapertures Nspot This figure is drawn by plotting the Nat value which gives the minimum residual wavefront error E for a given & value . Using this ...
Page 187
... figure are for D = 8 m and sense = 0.6 μm . For other D and Asense values , the values A , labeled to each line should be multiplied by [ sense / 0.6 μm ] [ 8 m / D ] . The curve for 8 = 0 is drawn by smoothly fitting the calculated ...
... figure are for D = 8 m and sense = 0.6 μm . For other D and Asense values , the values A , labeled to each line should be multiplied by [ sense / 0.6 μm ] [ 8 m / D ] . The curve for 8 = 0 is drawn by smoothly fitting the calculated ...
Page 402
... Figure 7 shows the relation between the color excess and co , the temperature index . The diagram is useful in seeing if there is any adverse correlation of the calibrations used as a function of temperature . None seems to be in ...
... Figure 7 shows the relation between the color excess and co , the temperature index . The diagram is useful in seeing if there is any adverse correlation of the calibrations used as a function of temperature . None seems to be in ...
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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray