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 102
... relative rotations , six relative offsets AX , and AY ,, and three relative scales , an We find n = ( 2 ) Figure 1 shows the relative orientation of the four CCD chips as given by Eq . ( 1 ) . The errors σ listed in Eq . ( 1 ) are ...
... relative rotations , six relative offsets AX , and AY ,, and three relative scales , an We find n = ( 2 ) Figure 1 shows the relative orientation of the four CCD chips as given by Eq . ( 1 ) . The errors σ listed in Eq . ( 1 ) are ...
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 ...
... 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 ...
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absorption abundance accretion analysis asteroids 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 pixel 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 stellar winds subgiant survey Table telescope temperature tion turnoff values variability wavelength white dwarf width X-ray XX Vir