Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 69
... effects are at once noticed in Fig . 2 where the identified clusters are shaded . Results are presented in Table 1 in sequential order . Column 1 gives the cluster number and column 2 records the number of members in the cluster . The ...
... effects are at once noticed in Fig . 2 where the identified clusters are shaded . Results are presented in Table 1 in sequential order . Column 1 gives the cluster number and column 2 records the number of members in the cluster . The ...
Page 196
... effects in Table 2. It is assumed that they arise in the crosscorrelation procedure . Measurement of the wavelengths of individual lines would not provide an independent test , since every broadened spectral feature is a blend of ...
... effects in Table 2. It is assumed that they arise in the crosscorrelation procedure . Measurement of the wavelengths of individual lines would not provide an independent test , since every broadened spectral feature is a blend of ...
Page 200
... effects of the diffusion of " He . Including the effects of helium diffusion has a negligible effect ( < 0.5 Gyr ) on the derived ages of globular clusters . Regardless of the inclusion of helium diffusion , a significant age spread of ...
... effects of the diffusion of " He . Including the effects of helium diffusion has a negligible effect ( < 0.5 Gyr ) on the derived ages of globular clusters . Regardless of the inclusion of helium diffusion , a significant age spread of ...
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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