Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 73
... bright point source ( Fig . 1 , row 3 ) . Removal of the bright source followed by deconvolution with the seeing , however , restores the elliptical shape of this object . 3.4 Arp 142 - NGC 2936 + 2937 Simulations employing this ...
... bright point source ( Fig . 1 , row 3 ) . Removal of the bright source followed by deconvolution with the seeing , however , restores the elliptical shape of this object . 3.4 Arp 142 - NGC 2936 + 2937 Simulations employing this ...
Page 201
... Bright Stars in Omega Centauri and the Type II Cepheid ST Puppis GUILLERMO GONZALEZ Thesis work conducted at : Department of Astronomy , University of Washington Current address : Department of Astronomy and McDonald Observatory ...
... Bright Stars in Omega Centauri and the Type II Cepheid ST Puppis GUILLERMO GONZALEZ Thesis work conducted at : Department of Astronomy , University of Washington Current address : Department of Astronomy and McDonald Observatory ...
Page 272
... bright ( V < 15.5 ) giants , whose flux - weighted mean apparent magnitude is 14.42 . If the giant branch as a whole is shifted to the blue by 0.1 mag ( 10 % ) compared to its outer - cluster counterpart , the 70 bright giants produce ...
... bright ( V < 15.5 ) giants , whose flux - weighted mean apparent magnitude is 14.42 . If the giant branch as a whole is shifted to the blue by 0.1 mag ( 10 % ) compared to its outer - cluster counterpart , the 70 bright giants produce ...
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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