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Page 63
Over half of the recovered objects were found to correspond to previously cataloged galaxies ; few if any of these are dwarf spheriodal galaxies , but rather mostly dwarf irregulars of low surface brightness ...
Over half of the recovered objects were found to correspond to previously cataloged galaxies ; few if any of these are dwarf spheriodal galaxies , but rather mostly dwarf irregulars of low surface brightness ...
Page 66
DISCUSSION The positions of dwarf galaxies originally collected by Mailyan ( 1973 ) have been substantially corrected , making it now possible to include them in the NED data base , and thereby permit a study of these objects in a ...
DISCUSSION The positions of dwarf galaxies originally collected by Mailyan ( 1973 ) have been substantially corrected , making it now possible to include them in the NED data base , and thereby permit a study of these objects in a ...
Page 115
The situation is compounded by unavoidable correlations between fundamental quantities such as redshift and luminosity in samples of objects obtained from flux - limited surveys . 2.1 Absolute Magnitudes and Luminosities The division in ...
The situation is compounded by unavoidable correlations between fundamental quantities such as redshift and luminosity in samples of objects obtained from flux - limited surveys . 2.1 Absolute Magnitudes and Luminosities The division in ...
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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