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 behavior of a quasar . This in turn will include at least two factors : time scale and amplitude , and these may not be separable . The amplitude and time scale of the variability exhibited by a quasar will also show a ...
... variability behavior of a quasar . This in turn will include at least two factors : time scale and amplitude , and these may not be separable . The amplitude and time scale of the variability exhibited by a quasar will also show a ...
Page 373
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . Primary significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 1 3.2 Eclipse Phase The polarimetric ...
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . Primary significance of the regions A and B ( Fig . 4 ) over a number of orbital cycles . 1 3.2 Eclipse Phase The polarimetric ...
Page 373
... variability increases during secondary eclipse . Variability decreases as primary eclipse progresses . -ד 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 . -ד 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 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