Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 105
... suggest that dust scattering is the dominant cause of the observed nuclear polarization . The corrected continuum ... suggests that F2 may represent the optically thin thermal radiation from the scattering region itself . Barring ...
... suggest that dust scattering is the dominant cause of the observed nuclear polarization . The corrected continuum ... suggests that F2 may represent the optically thin thermal radiation from the scattering region itself . Barring ...
Page 645
... suggests that it is being affected by radio jet interaction with a dense ISM in the host galaxy . A redirection of ... suggest that the galaxy is a fairly old merger . The small size of the radio source , the correspondence with the ...
... suggests that it is being affected by radio jet interaction with a dense ISM in the host galaxy . A redirection of ... suggest that the galaxy is a fairly old merger . The small size of the radio source , the correspondence with the ...
Page 874
... suggest for Fẞ ( 5 ) a mean error of ~ 15 % . 5. ON THE NATURE OF THE THREE OBJECTS He 2-111 is an extreme bipolar ... suggests , as stated by Peimbert and Torres - Peimbert ( 1983 ) , that the higher the N / O ratio the smaller the O ...
... suggest for Fẞ ( 5 ) a mean error of ~ 15 % . 5. ON THE NATURE OF THE THREE OBJECTS He 2-111 is an extreme bipolar ... suggests , as stated by Peimbert and Torres - Peimbert ( 1983 ) , that the higher the N / O ratio the smaller the O ...
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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