Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 141
... estimate of the statistical weight of that individual estimate of the mean adjustment . The weighted residuals to this adjustment are listed in the last column . The adjustment found for each region is based upon the luminosity ...
... estimate of the statistical weight of that individual estimate of the mean adjustment . The weighted residuals to this adjustment are listed in the last column . The adjustment found for each region is based upon the luminosity ...
Page 258
... estimate of the median sky brightness is derived , rather than a mode . ( Using some estimate of the mode of the pixel histogram as the sky - brightness statistic is intended to allow for asymmetric positive - only contamination of the ...
... estimate of the median sky brightness is derived , rather than a mode . ( Using some estimate of the mode of the pixel histogram as the sky - brightness statistic is intended to allow for asymmetric positive - only contamination of the ...
Page 470
... estimate the relative frequency of the W UMa systems in these populous clusters by simply adding numbers of monitored stars and of discovered W UMa's in the three clusters and take global ratios . We note that distance moduli of these ...
... estimate the relative frequency of the W UMa systems in these populous clusters by simply adding numbers of monitored stars and of discovered W UMa's in the three clusters and take global ratios . We note that distance moduli of these ...
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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