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 contam- ination of ...
... 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 contam- ination of ...
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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Common terms and phrases
absorption abundance accretion analysis asteroids Astronomical Society binary bright calibration catalog central star chromospheric clouds color comets correction derived detection detector diagram disk distribution eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular clusters H II regions Hyades indices infrared ionized km s¹ light curve lines luminosity magnitude main sequence main-sequence mass measured MNRAS objects observations Observatory obtained open clusters optical orbital parameters PASP period phase photometric pixel planetary nebulae plotted quasars radial velocities radius range ratio red giants reddening redshift region residuals rotation sample scale scatter secondary solar sources spectral type spectroscopic spectrum standard stellar stellar winds subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir