Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 102
... scatter which takes account of the finite resolution and any other unrecognized sources of error . The cosmic scatter was determined by requiring that the x2 per degree of freedom be unity , and was found to be 0.044 ground - based ...
... scatter which takes account of the finite resolution and any other unrecognized sources of error . The cosmic scatter was determined by requiring that the x2 per degree of freedom be unity , and was found to be 0.044 ground - based ...
Page 398
... scatter than for the brightest stars . A comparison of the present data to that in the three papers referenced above containing previously published uvby data is given in Table 2. Obviously , there are significant differences between ...
... scatter than for the brightest stars . A comparison of the present data to that in the three papers referenced above containing previously published uvby data is given in Table 2. Obviously , there are significant differences between ...
Page 459
... scatter in this plot catches one's eye at once . To analyze this scatter , a regression of RG on is useful . The relation which results from one - error leastsquares analysis is ( 7 ) If residuals R ( R ) from this equation are plotted ...
... scatter in this plot catches one's eye at once . To analyze this scatter , a regression of RG on is useful . The relation which results from one - error leastsquares analysis is ( 7 ) If residuals R ( R ) from this equation are plotted ...
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absorption abundance accretion analysis asteroids astrometry 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 pixels 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 subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir