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 86
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 ...
Other editions - View all
Common terms and phrases
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