Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 160
... shown as solid dots labeled with the final four digits of their GSC numbers . Other GSC stars are shown as open circles . The position of the nucleus is shown by the cross at the center of the figure , while the position of SN 1993J is ...
... shown as solid dots labeled with the final four digits of their GSC numbers . Other GSC stars are shown as open circles . The position of the nucleus is shown by the cross at the center of the figure , while the position of SN 1993J is ...
Page 166
... shown in Fig . 3 is the sum of the four spectra given in Fig . 2. The observed data are displayed by asterisks and the residuals are shown at the bottom by dotted lines . The observed profile with a signal to noise ratio , S / N ~ 40 ...
... shown in Fig . 3 is the sum of the four spectra given in Fig . 2. The observed data are displayed by asterisks and the residuals are shown at the bottom by dotted lines . The observed profile with a signal to noise ratio , S / N ~ 40 ...
Page 532
... shown in Fig . 1 , and one of these defects is shown on an expanded scale in Fig . 2 ( a ) . As a result of the way the charge collected in a pixel is transferred along a column , an electron trap usually causes a reduction in the ...
... shown in Fig . 1 , and one of these defects is shown on an expanded scale in Fig . 2 ( a ) . As a result of the way the charge collected in a pixel is transferred along a column , an electron trap usually causes a reduction in the ...
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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