Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 71
... galaxies . To test the power of this technique , we synthesize the appearance of QSOS at z = 0.3 by combining bright stellar profiles and artificially redshifted images of seven nearby , luminous galaxies with interesting morphology ...
... galaxies . To test the power of this technique , we synthesize the appearance of QSOS at z = 0.3 by combining bright stellar profiles and artificially redshifted images of seven nearby , luminous galaxies with interesting morphology ...
Page 72
Galaxy NGC 5194 2936 + 37 4486 5257 + 58 2623 5426 + 27 2832 Galaxy Arp 85 142 152 240 243 271 315 TABLE 1 Model Host Galaxies Distancea Bolometric Flux ( Mpc ) Magnitudea Reduction 7.7 -96 16.8 ~ 94 77 -36 95 -20.75 -20.6 -21.64 -21.7 ...
Galaxy NGC 5194 2936 + 37 4486 5257 + 58 2623 5426 + 27 2832 Galaxy Arp 85 142 152 240 243 271 315 TABLE 1 Model Host Galaxies Distancea Bolometric Flux ( Mpc ) Magnitudea Reduction 7.7 -96 16.8 ~ 94 77 -36 95 -20.75 -20.6 -21.64 -21.7 ...
Page 170
... galaxies with observed type Ia supernovae have been identified in each of three Lyon groups of galaxies not associated ... galaxies common to both methods listed in Table 2 of Garcia ( 1993 ) . The inclusion of the galaxies in the Lyon ...
... galaxies with observed type Ia supernovae have been identified in each of three Lyon groups of galaxies not associated ... galaxies common to both methods listed in Table 2 of Garcia ( 1993 ) . The inclusion of the galaxies in the Lyon ...
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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