Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 38
... sources are discussed , and finding charts are included for all sources listed . Additionally , follow - up spectroscopic and positional information is provided for several objects first listed in Paper I of this series . One new ...
... sources are discussed , and finding charts are included for all sources listed . Additionally , follow - up spectroscopic and positional information is provided for several objects first listed in Paper I of this series . One new ...
Page 846
... sources > 15 ′ from field center errors may be larger All values are background subtracted count rates using an aperture of 25 " diameter d From TABle 1 e Angular distance of the source from center of field These sources have < 30 ...
... sources > 15 ′ from field center errors may be larger All values are background subtracted count rates using an aperture of 25 " diameter d From TABle 1 e Angular distance of the source from center of field These sources have < 30 ...
Page 847
... sources ( Long et al . 1981 ) , W = Wang et al . ( 1991 ) sources Einstein coordinates , precessed to 2000.0 All values are background subtracted count rates using a 100 " diameter aperture From Table 1 Based on Einstein - IPC intensity ...
... sources ( Long et al . 1981 ) , W = Wang et al . ( 1991 ) sources Einstein coordinates , precessed to 2000.0 All values are background subtracted count rates using a 100 " diameter aperture From Table 1 Based on Einstein - IPC intensity ...
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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