Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 286
... included . Based upon their motions , stars were assigned to one of four classes : class 1 = definite membership ; class 2 = probable membership ; class 3 = probable nonmembership ; and class 4 = definite nonmembership . Column 3 of ...
... included . Based upon their motions , stars were assigned to one of four classes : class 1 = definite membership ; class 2 = probable membership ; class 3 = probable nonmembership ; and class 4 = definite nonmembership . Column 3 of ...
Page 491
... included ; stars brighter than_V = 17.0_are included even if m , or Hẞ was not derived . We have constructed a synthetic finding chart in Fig . 4 . based on the date in Table 3 and its extension to fainter magnitudes . The size and type ...
... included ; stars brighter than_V = 17.0_are included even if m , or Hẞ was not derived . We have constructed a synthetic finding chart in Fig . 4 . based on the date in Table 3 and its extension to fainter magnitudes . The size and type ...
Page 824
... included as a standard for comparison . 8600 troduced by the placement of the local continuum . We estimate this error to be ± 10 % of the tabulated values . Eps Cyg 3. RESULTS We discuss individual stars below and summarize the results ...
... included as a standard for comparison . 8600 troduced by the placement of the local continuum . We estimate this error to be ± 10 % of the tabulated values . Eps Cyg 3. RESULTS We discuss individual stars below and summarize the results ...
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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