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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absorption abundance accretion analysis asteroids astrometry Astronomical Society binary bright calibration catalog central star chromospheric clouds color comets correction derived detection detector diagram disk distribution eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular clusters H II regions Hyades indices infrared ionized km s¹ light curve lines luminosity magnitude main sequence main-sequence mass measured MNRAS objects observations Observatory obtained open clusters optical orbital parameters PASP period phase photometric pixels planetary nebulae plotted quasars radial velocities radius range ratio red giants reddening redshift region residuals rotation sample scale scatter secondary solar sources spectral type spectroscopic spectrum standard stellar subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir