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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abundance additional analysis appear associations assumed Astronomical average binary blue bright calibration catalog central clouds cluster color compared correction derived detection determined discussed distance distribution dwarf eclipse effects emission errors estimate et al evidence evolution field Figure flux frame function galaxies giants given groups included increase indices less light limit lines luminosity magnitude mass mean measured MNRAS nebulae noted objects observations obtained optical orbital PASP period phase photometric pixels position possible present probably quasars range ratio reduced reference region relation relative rotation sample scale scatter secondary shown similar sources spectral spectrum standard stars stellar stellar winds suggests surface survey Table telescope temperature tion University values variability velocity wavelength X-ray