Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 373
... Phase The polarimetric variability during eclipse phase has been investigated for some binary systems to detect the possible presence of limb polarization ( Pirrola 1980 ; Kemp et al . 1983 ) and to probe the envelope geometry ( St ...
... Phase The polarimetric variability during eclipse phase has been investigated for some binary systems to detect the possible presence of limb polarization ( Pirrola 1980 ; Kemp et al . 1983 ) and to probe the envelope geometry ( St ...
Page 861
... Phase Wavelength ( Å ) FIG . 6 Emission - line flux from individual HL CMa spectra vs orbital phase , C Iv 1550 Å ( * ) and Si IV 1394 Å ( + ) . that the system not only went into outburst but had reached maximum four days following ...
... Phase Wavelength ( Å ) FIG . 6 Emission - line flux from individual HL CMa spectra vs orbital phase , C Iv 1550 Å ( * ) and Si IV 1394 Å ( + ) . that the system not only went into outburst but had reached maximum four days following ...
Page 866
... Phase 0 8 10 1.5 Si III 1299 2 ( 10- " ergs cm " s " ' ) Al III 1857 1.0F 0.5 FIG . 21 - C IV 1550 Å ( * ) and Si Iv ... phase 0.4 through phase 0.7 . The F ( 10 ergs cm " s " ) Fx ( 10 ergs cm " s " ) 20 20 CNV 1550 15 10 F ( 10 " ergs ...
... Phase 0 8 10 1.5 Si III 1299 2 ( 10- " ergs cm " s " ' ) Al III 1857 1.0F 0.5 FIG . 21 - C IV 1550 Å ( * ) and Si Iv ... phase 0.4 through phase 0.7 . The F ( 10 ergs cm " s " ) Fx ( 10 ergs cm " s " ) 20 20 CNV 1550 15 10 F ( 10 " ergs ...
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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