Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 382
... wavelength region from 3800 to 4800 Å , initially used for the MK classification scheme , has been extended to shorter wavelengths through space technology . The UV range has been included in the classification schemes thanks to ...
... wavelength region from 3800 to 4800 Å , initially used for the MK classification scheme , has been extended to shorter wavelengths through space technology . The UV range has been included in the classification schemes thanks to ...
Page 569
... WAVELENGTH ........ 8000 8000 1 1 7000 9000 WAVELENGTH ( ANGSTROMS ) FIG . 6 - Comparison between the new CTIO monochromatic fluxes and Baldwin and Stone's ( 1984 ) measurements , in the sense of CTIO minus Baldwin and Stone , plotted ...
... WAVELENGTH ........ 8000 8000 1 1 7000 9000 WAVELENGTH ( ANGSTROMS ) FIG . 6 - Comparison between the new CTIO monochromatic fluxes and Baldwin and Stone's ( 1984 ) measurements , in the sense of CTIO minus Baldwin and Stone , plotted ...
Page 740
... wavelength . The errors in position angle are as given in Table 1. The errors in wavelength represent the bandwidth of the filter used in the imaging . The three lines in each case represent the best - fit line as well as the ± lo ...
... wavelength . The errors in position angle are as given in Table 1. The errors in wavelength represent the bandwidth of the filter used in the imaging . The three lines in each case represent the best - fit line as well as the ± lo ...
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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