Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 371
... appears to be several significant peaks , with one strong peak with a period of 1 day being possibly a third harmonic of the orbital period , as predicted by Brown et al . ( 1982 ) . However , as periods of 1 day sometimes appear in ...
... appears to be several significant peaks , with one strong peak with a period of 1 day being possibly a third harmonic of the orbital period , as predicted by Brown et al . ( 1982 ) . However , as periods of 1 day sometimes appear in ...
Page 373
... appears to be several significant peaks , with one strong peak with a period of 1 day being possibly a third harmonic of the orbital period , as predicted by Brown et al . ( 1982 ) . However , as periods of 1 day sometimes appear in ...
... appears to be several significant peaks , with one strong peak with a period of 1 day being possibly a third harmonic of the orbital period , as predicted by Brown et al . ( 1982 ) . However , as periods of 1 day sometimes appear in ...
Page 675
... appear elongated over scales of ~ 5 " -10 " from the image core . This elongation has been attributed to errors in the attitude correction as the satellite is wobbled during the observations , and affects sources with both soft and hard ...
... appear elongated over scales of ~ 5 " -10 " from the image core . This elongation has been attributed to errors in the attitude correction as the satellite is wobbled during the observations , and affects sources with both soft and hard ...
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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