Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 133
... light curve is single or double wave , or possibly 1.08 days ( Bossi and Guerrero 1989 ) . It should be kept in mind ... light curves , that the most satisfactory photometric period was 0.665 day ( or twice this value if the light ...
... light curve is single or double wave , or possibly 1.08 days ( Bossi and Guerrero 1989 ) . It should be kept in mind ... light curves , that the most satisfactory photometric period was 0.665 day ( or twice this value if the light ...
Page 152
V Light 0.4 0.6 0.8 1.0 B 0.6 0.8 1.0 1.2 B Light 0.2 -0.2 0.0 0.2 0.4 0.6 0.4 0.8 Phase 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 0.4 0.6 0.8 1.0 B 0.6 0.8 1.0 1.2 B Light 0.2 -0.2 0.0 0.2 0.4 0.6 0.4 0.8 Phase 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 882
... light curve . Krolik et al . ( 1991 ) show a PDS computed from the IUE data for NGC 5548 from Clavel et al . ( 1991 ) ... light curves . We generate model continua by assuming that the PDS can be modeled as a power law , and carry ...
... light curve . Krolik et al . ( 1991 ) show a PDS computed from the IUE data for NGC 5548 from Clavel et al . ( 1991 ) ... light curves . We generate model continua by assuming that the PDS can be modeled as a power law , and carry ...
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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