Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 38
... 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 cataclysmic ...
... 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 cataclysmic ...
Page 479
... discussed above suggest the Q values of stars of similar period may be different . Nevertheless , the P√p = Q relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is ...
... discussed above suggest the Q values of stars of similar period may be different . Nevertheless , the P√p = Q relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is ...
Page 793
... discussed the present status of attempts to confront these expectations with observations of supernova remnants . The bottom line is that there is presently no convincing evidence that real supernova remnants have cosmic - ray ...
... discussed the present status of attempts to confront these expectations with observations of supernova remnants . The bottom line is that there is presently no convincing evidence that real supernova remnants have cosmic - ray ...
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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