Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 400
... value of E ( b - y ) = 0.54 mag . This value is equivalent to a E ( B – V ) of about 0.75 , close to the values obtained by others previ- ously . The standard deviation is not much larger than one would expect from observational errors ...
... value of E ( b - y ) = 0.54 mag . This value is equivalent to a E ( B – V ) of about 0.75 , close to the values obtained by others previ- ously . The standard deviation is not much larger than one would expect from observational errors ...
Page 477
... values . Although the Teff values at maximum and minimum light differ by ~ 200 K from the values originally derived by Alexander et al . ( 1987 ) , the new mean values ( ( Teff ) = 6690 K , ( log g ) = 2.37 ) differ only slightly from ...
... values . Although the Teff values at maximum and minimum light differ by ~ 200 K from the values originally derived by Alexander et al . ( 1987 ) , the new mean values ( ( Teff ) = 6690 K , ( log g ) = 2.37 ) differ only slightly from ...
Page 479
... values of stars of similar period may be different . Nevertheless , the P√p = Q relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is indeed the case and write the P ...
... values of stars of similar period may be different . Nevertheless , the P√p = Q relation should be valid in the mean in view of the P - L relation exhibited by the variable stars . We assume that this is indeed the case and write the P ...
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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