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 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 866
... phase 0.4 through phase 0.7 . The 0.0 0.5 00 C IV 1550 Orbital Phase 0.2 0.4 06 0.8 1.0 Orbital Phase Si III 1299 02 1.0 04 08 0.6 Orbita Phase 10 F ( 10 " ergs cm2 s " 1 ) ( 10 ergs cm2 s1 ) t 00 0.0 2.0 15 1.5 00 * Si NV 1394 2.0 0.2 ...
... phase 0.4 through phase 0.7 . The 0.0 0.5 00 C IV 1550 Orbital Phase 0.2 0.4 06 0.8 1.0 Orbital Phase Si III 1299 02 1.0 04 08 0.6 Orbita Phase 10 F ( 10 " ergs cm2 s " 1 ) ( 10 ergs cm2 s1 ) t 00 0.0 2.0 15 1.5 00 * Si NV 1394 2.0 0.2 ...
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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray