Publications of the Astronomical Society of the Pacific, Volume 106, Issues 695-702Astronomical Society of the Pacific, 1994 |
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Page 49
... GCLF results if a2-1 = 1 - ap and a2 = a1 . In short , with ao < 1 and a1 , a2 > 1 , a GCLF can be symmetric about its peak Mv , 1 if and only if 1 - a = a1 - 1 = a2-1 , i.e. , if | 1 - a ( L ) | = constant . ( 9 ) Note that this is ...
... GCLF results if a2-1 = 1 - ap and a2 = a1 . In short , with ao < 1 and a1 , a2 > 1 , a GCLF can be symmetric about its peak Mv , 1 if and only if 1 - a = a1 - 1 = a2-1 , i.e. , if | 1 - a ( L ) | = constant . ( 9 ) Note that this is ...
Page 50
... GCLF ( dots ) . This example was calcu- lated through Eq . ( 7 ) , assuming | 1 - a ( L ) | = 0.2 , Lmin = 102L , L1 = 8 × 10 * L , L2 = Lmax = 6.4 × 107 Lo , a total population of 200 , and a bin width of 0.1 mag . The solid line is ...
... GCLF ( dots ) . This example was calcu- lated through Eq . ( 7 ) , assuming | 1 - a ( L ) | = 0.2 , Lmin = 102L , L1 = 8 × 10 * L , L2 = Lmax = 6.4 × 107 Lo , a total population of 200 , and a bin width of 0.1 mag . The solid line is ...
Page 53
... GCLF is perhaps better reproduced with a0 = 0 and a1 = 2 ; then the GCLF is expected to be slightly narrower than the Galactic distribution ( with a = 0.15 ) , which is indeed found ( Secker 1992 ) . The important point of Figs . 5 and ...
... GCLF is perhaps better reproduced with a0 = 0 and a1 = 2 ; then the GCLF is expected to be slightly narrower than the Galactic distribution ( with a = 0.15 ) , which is indeed found ( Secker 1992 ) . The important point of Figs . 5 and ...
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absorption abundance accretion analysis arcsec asteroids Astronomical Society binary bright calibration catalog central star chromospheric clouds cluster color comets correction derived detection detector diagram disk Dordrecht eclipse emission errors estimate evolution expansion velocities Fe/H field flux frame function galactic galaxies GCLF giant branch globular globular clusters H II regions Hyades indices infrared ionized km s¯¹ lines luminosity m₁ magnitude main sequence main-sequence mass measured MNRAS objects Observatory observed 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 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