Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 75
... possible to discriminate between an underlying disk and an elliptical host galaxy solely by examining the outer regions of the brightness profiles of the subtraction residuals . More significantly , the mean recovery of a host galaxy's ...
... possible to discriminate between an underlying disk and an elliptical host galaxy solely by examining the outer regions of the brightness profiles of the subtraction residuals . More significantly , the mean recovery of a host galaxy's ...
Page 214
... Possible 511 KeV emission ( Briggs et al . 1991 ) . RE 0751 + 144 . Periodic variations in circular and linear polarization in VRI , suggesting Bwd = 8-18 MG ( 41 ) . Possible subharmonic at 1667 s . BG CMi . Circular polarization in I ...
... Possible 511 KeV emission ( Briggs et al . 1991 ) . RE 0751 + 144 . Periodic variations in circular and linear polarization in VRI , suggesting Bwd = 8-18 MG ( 41 ) . Possible subharmonic at 1667 s . BG CMi . Circular polarization in I ...
Page 374
... possible geometries for the scattering envelope of Y Cyg , though offered little evidence to support their speculations . In summary they suggested : ( i ) A possibly small phase - locked second - harmonic variation may be present in ...
... possible geometries for the scattering envelope of Y Cyg , though offered little evidence to support their speculations . In summary they suggested : ( i ) A possibly small phase - locked second - harmonic variation may be present in ...
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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