Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 246
... measured by Wright were usable . Lines were identified on the tracings with the aid of Davis ' ( 1947 ) identification of the spectrum of ẞ Pegasi . Lines denoted as blended in that reference were not measured . Many additional lines ...
... measured by Wright were usable . Lines were identified on the tracings with the aid of Davis ' ( 1947 ) identification of the spectrum of ẞ Pegasi . Lines denoted as blended in that reference were not measured . Many additional lines ...
Page 322
... measured values . The fits ( boxes ) to the measured minima ( diamonds ) for the QDSS data are worse than those of the FOE data or the SSS data . The QDSS has noticeable ghost orders which complicate accurate determination of the data ...
... measured values . The fits ( boxes ) to the measured minima ( diamonds ) for the QDSS data are worse than those of the FOE data or the SSS data . The QDSS has noticeable ghost orders which complicate accurate determination of the data ...
Page 501
... measured from [ O III ] tends to be higher than the expansion velocity as measured from the Balmer lines . 50 It is consequently seen that there is sometimes a significant difference in the velocity estimates as determined by ...
... measured from [ O III ] tends to be higher than the expansion velocity as measured from the Balmer lines . 50 It is consequently seen that there is sometimes a significant difference in the velocity estimates as determined by ...
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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