Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 135
... lines can be used for the solution of the inverse problem , that seemed inappropriate here . The observed lines are quite shallow . The identifications of some of the blending lines are uncertain , which does not allow us to treat them ...
... lines can be used for the solution of the inverse problem , that seemed inappropriate here . The observed lines are quite shallow . The identifications of some of the blending lines are uncertain , which does not allow us to treat them ...
Page 246
... lines measured by Wright were usable . Lines were identified on the tracings with the aid of Davis ' ( 1947 ) identification of the spectrum of ẞ Pegasi . Lines denoted as blended in that reference were not measured . Many addi- tional ...
... lines measured by Wright were usable . Lines were identified on the tracings with the aid of Davis ' ( 1947 ) identification of the spectrum of ẞ Pegasi . Lines denoted as blended in that reference were not measured . Many addi- tional ...
Page 877
... lines and extremely broad emission features , es- pecially at the He II lines . Identifications for some lines are marked . 1-5 1991 give V = 15.585 ± 0.011 . There are just two images each in U and B , but they yield ( B - V ) = + ...
... lines and extremely broad emission features , es- pecially at the He II lines . Identifications for some lines are marked . 1-5 1991 give V = 15.585 ± 0.011 . There are just two images each in U and B , but they yield ( B - V ) = + ...
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absorption abundance accretion analysis asteroids 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 pixel 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 stellar winds subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir