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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absorption abundance accretion analysis asteroids astrometry Astronomical Society binary bright calibration catalog central star chromospheric clouds color comets correction derived detection detector diagram disk distribution eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular clusters H II regions Hyades indices infrared ionized km s¹ light curve lines luminosity magnitude main sequence main-sequence mass measured MNRAS objects observations Observatory obtained open clusters optical orbital parameters PASP period phase photometric pixels planetary nebulae plotted quasars radial velocities radius range ratio red giants reddening redshift region residuals rotation sample scale scatter secondary solar sources spectral type spectroscopic spectrum standard stellar subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir