Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 101
... relative to one another by up to 1 ° . The solution is based on images taken between December 1990 and June 1992 and is stable over that entire period . We also present a solution for the relative positions and orientations of the four ...
... relative to one another by up to 1 ° . The solution is based on images taken between December 1990 and June 1992 and is stable over that entire period . We also present a solution for the relative positions and orientations of the four ...
Page 103
... relative angles , 4 , and relative scales , a ,, in Eq . ( 4 ) are in very good agreement with those given by Monet based on observations of @ Cen and NGC 1850 ( Faber 1991 ) . The offsets AX , and AY , differ from those given by Monet ...
... relative angles , 4 , and relative scales , a ,, in Eq . ( 4 ) are in very good agreement with those given by Monet based on observations of @ Cen and NGC 1850 ( Faber 1991 ) . The offsets AX , and AY , differ from those given by Monet ...
Page 385
... relative . In order to convert to flux the intensity axis should be multiplied by 10-13 erg cm2 s - 1 Å - 1 . The data are affected by seeing and transparency variations , but can always be converted from relative flux to absolute flux ...
... relative . In order to convert to flux the intensity axis should be multiplied by 10-13 erg cm2 s - 1 Å - 1 . The data are affected by seeing and transparency variations , but can always be converted from relative flux to absolute flux ...
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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