Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 149
... light were determined and an improved ephemeris is given . Analysis of the observations with the latest version of the WilsonDevinney program shows that the system is semidetached . Our solution does not indicate the presence of third light ...
... light were determined and an improved ephemeris is given . Analysis of the observations with the latest version of the WilsonDevinney program shows that the system is semidetached . Our solution does not indicate the presence of third light ...
Page 152
V Light 1.0 0.8 0.6 0.4 0.2 V Light 1.0 0.8 0.6 -0.2 0.4 0.0 0.2 0.2 -0.2 Phase 0.0 0.4 FIG . 1 - DHK observations of XZ CMi in the B and V bandpasses with the computed curve from the elements of Table 4 . be done , one including third ...
V Light 1.0 0.8 0.6 0.4 0.2 V Light 1.0 0.8 0.6 -0.2 0.4 0.0 0.2 0.2 -0.2 Phase 0.0 0.4 FIG . 1 - DHK observations of XZ CMi in the B and V bandpasses with the computed curve from the elements of Table 4 . be done , one including third ...
Page 153
V Light 1.0 0.8 0.6 0.4 0.2 V Light 1.0 0.8 0.6 -0.2 0.4 0.2 0.0 0.2 -0.2 Phase 0.0 0.4 FIG . 1 - DHK observations of XZ CMi in the B and V bandpasses with the computed curve from the elements of Table 4 . be done , one including third ...
V Light 1.0 0.8 0.6 0.4 0.2 V Light 1.0 0.8 0.6 -0.2 0.4 0.2 0.0 0.2 -0.2 Phase 0.0 0.4 FIG . 1 - DHK observations of XZ CMi in the B and V bandpasses with the computed curve from the elements of Table 4 . be done , one including third ...
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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