Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 16
... less information during smoothing than other methods in current use . This information - conserving aspect makes wavelet transforms a particularly promising approach to the problem of data archiving and storage ( Richter 1994 ; Bijaoui ...
... less information during smoothing than other methods in current use . This information - conserving aspect makes wavelet transforms a particularly promising approach to the problem of data archiving and storage ( Richter 1994 ; Bijaoui ...
Page 302
... less than 0.7 for the coolest . The Li dip is readily apparent starting sharply at ( B - V ) = 0.42 and merging with the more gradual Li depletion on the cool side near ( B - V ) = 0.54 . The results from NGC 752 can shed some light on ...
... less than 0.7 for the coolest . The Li dip is readily apparent starting sharply at ( B - V ) = 0.42 and merging with the more gradual Li depletion on the cool side near ( B - V ) = 0.54 . The results from NGC 752 can shed some light on ...
Page 406
... less than 0.050 mag , and B - V errors less than 0.071 mag are shown in Fig . 2 and Table 2. In limiting ourselves to these stars , we ensure that only the highest quality photometry is included in the CMD . Figure 3 shows the CMD for ...
... less than 0.050 mag , and B - V errors less than 0.071 mag are shown in Fig . 2 and Table 2. In limiting ourselves to these stars , we ensure that only the highest quality photometry is included in the CMD . Figure 3 shows the CMD for ...
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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