Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 276
... plotted the same set of blue HB and EHB stars with large filled sym- bols , to allow their use as a navigational aid in the unfa- miliar ultraviolet diagrams . The brightest giants , with V ~ 13-13.5 , may be used for the same purpose ...
... plotted the same set of blue HB and EHB stars with large filled sym- bols , to allow their use as a navigational aid in the unfa- miliar ultraviolet diagrams . The brightest giants , with V ~ 13-13.5 , may be used for the same purpose ...
Page 390
... plotted against spectral type for luminosity classes from I to V. It is clear that supergiants are easily ... plotted vs. spectral type , showing that the line is a luminosity indicator with a be- havior similar to Ha , as shown in ...
... plotted against spectral type for luminosity classes from I to V. It is clear that supergiants are easily ... plotted vs. spectral type , showing that the line is a luminosity indicator with a be- havior similar to Ha , as shown in ...
Page 729
... plotted against V ; ( b ) residual in b is plotted against V ; ( c ) residual in v is plotted against B - V ; ( d ) residual in b is plotted against B - V ; ( e ) and ( f ) residuals in v and bare plotted against airmass both for ...
... plotted against V ; ( b ) residual in b is plotted against V ; ( c ) residual in v is plotted against B - V ; ( d ) residual in b is plotted against B - V ; ( e ) and ( f ) residuals in v and bare plotted against airmass both for ...
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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