Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 125
... variability properties . For exam- ple , should one component of the quasar SED ( say the underlying power law ) vary on a different time scale than the Big Blue Bump , then the variability properties of qua- sars will show a dependence ...
... variability properties . For exam- ple , should one component of the quasar SED ( say the underlying power law ) vary on a different time scale than the Big Blue Bump , then the variability properties of qua- sars will show a dependence ...
Page 373
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 3.2 Eclipse Phase The polarimetric variability ...
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 3.2 Eclipse Phase The polarimetric variability ...
Page 373
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 3.2 Eclipse Phase The polarimetric variability ...
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 3.2 Eclipse Phase The polarimetric variability ...
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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