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 addi- tional 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 addi- tional 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 via hydrogen Balmer lines , as these lines are usually much weaker than the [ O III ] lines in PNe and hence nebulae with measured Balmer emission tend to be large and bright . - - 1 = 9.5 The majority of published expansion ...
... measured via hydrogen Balmer lines , as these lines are usually much weaker than the [ O III ] lines in PNe and hence nebulae with measured Balmer emission tend to be large and bright . - - 1 = 9.5 The majority of published expansion ...
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absorption abundance accretion analysis asteroids 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 pixel 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 stellar winds subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir