Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 248
... obtained closer to the limb . McLaughlin ( 1952 ) estimated AEI values for plates obtained at very nearly the same times as these two observations of Wright's . On three ingress plates spanning △ = 1.6– 1.7 d , he determined an AEI of ...
... obtained closer to the limb . McLaughlin ( 1952 ) estimated AEI values for plates obtained at very nearly the same times as these two observations of Wright's . On three ingress plates spanning △ = 1.6– 1.7 d , he determined an AEI of ...
Page 623
... obtained by the use of these ICF and the ions listed at the foot of the table . The He * lines have been corrected for collisional effects following the procedure given by Peimbert and Torres - Peimbert ( 1987 ) with partial collisional ...
... obtained by the use of these ICF and the ions listed at the foot of the table . The He * lines have been corrected for collisional effects following the procedure given by Peimbert and Torres - Peimbert ( 1987 ) with partial collisional ...
Page 683
... obtained during an interval △ t ; around instants t ,; if △ ¡ « At¡¡ we obtain the same conditions of three single data . Supposing the three observations exactly match a constant period P , the following relationship holds : n = This ...
... obtained during an interval △ t ; around instants t ,; if △ ¡ « At¡¡ we obtain the same conditions of three single data . Supposing the three observations exactly match a constant period P , the following relationship holds : n = This ...
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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