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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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