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 73
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 ...
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