Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
From inside the book
Results 1-3 of 82
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 ...
Other editions - View all
Common terms and phrases
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