Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 60
... orbital decay time -1/4 - 1/8 a Tam = -4.8x10 ° ( 102 ) ( M ) ( 0.25M ) Tdec = L L 9/8 " 49/8 yr . 49 t == ( 1-1 / 82 ao 8 Tdec ( 40 ) X ( 4 ) 5R Equation ( 4.3 ) of Zahn ( 1977 ) , with the same values for the physical variables ...
... orbital decay time -1/4 - 1/8 a Tam = -4.8x10 ° ( 102 ) ( M ) ( 0.25M ) Tdec = L L 9/8 " 49/8 yr . 49 t == ( 1-1 / 82 ao 8 Tdec ( 40 ) X ( 4 ) 5R Equation ( 4.3 ) of Zahn ( 1977 ) , with the same values for the physical variables ...
Page 861
... orbital period each night . Therefore , it is possible that the changes is the emission lines are due to an orbital modulation . Indeed , Fig . 6 , which shows the CIV 1550 Å and Si IV 1394 Å emission - line flux from the individual ...
... orbital period each night . Therefore , it is possible that the changes is the emission lines are due to an orbital modulation . Indeed , Fig . 6 , which shows the CIV 1550 Å and Si IV 1394 Å emission - line flux from the individual ...
Page 866
... orbital period . 1992 November data . However , there just is not enough archival data available to make any conclusions one way or another . Therefore , we still do not know if the C rv 1550 Å line flux variation we observed was a ...
... orbital period . 1992 November data . However , there just is not enough archival data available to make any conclusions one way or another . Therefore , we still do not know if the C rv 1550 Å line flux variation we observed was a ...
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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