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 566
... wavelength range permitted by the CCDs and to measure new fainter standards . In a previous paper ( Hamuy et al . 1992 ; hereafter Paper I ) we presented our results for the wavelength range 3300-7550 Å . As an extension of that work ...
... wavelength range permitted by the CCDs and to measure new fainter standards . In a previous paper ( Hamuy et al . 1992 ; hereafter Paper I ) we presented our results for the wavelength range 3300-7550 Å . As an extension of that work ...
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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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