FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1989219210> ?p ?o ?g. }

• W1989219210 endingPage "802" @default.
• W1989219210 startingPage "778" @default.
• W1989219210 abstract "This investigation presents a set of transformations to Johnson B-V, Cousins V-R, and Cousins V-I, as well as bolometric corrections to V, for [Fe/H] = -3, -2, -1, -0.5, 0.0, and +0.3 and, in each case, values of log g from -0.5 to 5.0 for 3000 K ≤ Teff ≤ 5500 K and from 2.0 to 5.0 for 6000 K ≤ Teff ≤ 40,000 K. These transformations employ the predictions from Kurucz model atmospheres at high temperatures (Teff ≥ 8000 K) and from MARCS model atmospheres at intermediate temperatures (from 7000 K down to a temperature in the range 4000 K ≤ Teff ≤ 5500 K, depending on [Fe/H], where adjustments to satisfy observational constraints become necessary). Thus, theoretical color-Teff relations are used exclusively down to a minimum temperature that is cooler than the temperatures of turnoff stars in open and globular star clusters. To better represent the color transformations obeyed by cool stars (down to 3000 K), corrections to the synthetic transformations have been determined from a careful consideration of observations for a few globular clusters (M92, M68, and 47 Tucanae), the color-magnitude diagrams (CMDs) of several open clusters (M67, the Pleiades, the Hyades, and NGC 6791), the CMDs and mass-luminosity diagram for solar neighborhood stars having good distance measurements from Hipparcos, empirical (B-V)-Teff and (V-K)-Teff relations, and color-color diagrams for field giants. The semiempirical color transformations that have been produced as a result of our analysis are also compared with several others that have been published in recent years: some of the deficiencies of the latter are revealed." @default.
• W1989219210 created "2016-06-24" @default.
• W1989219210 creator A5035340880 @default.
• W1989219210 creator A5038175562 @default.
• W1989219210 date "2003-08-01" @default.
• W1989219210 modified "2023-09-26" @default.
• W1989219210 title "Empirically Constrained Color-Temperature Relations. I.<i>BV</i>(<i>RI</i>)_C" @default.
• W1989219210 cites W1569860697 @default.
• W1989219210 cites W1588316676 @default.
• W1989219210 cites W1658485765 @default.
• W1989219210 cites W1840908835 @default.
• W1989219210 cites W195592436 @default.
• W1989219210 cites W1963828161 @default.
• W1989219210 cites W1966714030 @default.
• W1989219210 cites W1967378902 @default.
• W1989219210 cites W1976173770 @default.
• W1989219210 cites W1979186709 @default.
• W1989219210 cites W1979271265 @default.
• W1989219210 cites W1980350013 @default.
• W1989219210 cites W1982365042 @default.
• W1989219210 cites W1983853672 @default.
• W1989219210 cites W1989522864 @default.
• W1989219210 cites W1990702641 @default.
• W1989219210 cites W1991350869 @default.
• W1989219210 cites W1993681724 @default.
• W1989219210 cites W1998708134 @default.
• W1989219210 cites W1999645097 @default.
• W1989219210 cites W2000852443 @default.
• W1989219210 cites W2001869299 @default.
• W1989219210 cites W2003115978 @default.
• W1989219210 cites W2011810912 @default.
• W1989219210 cites W2019482685 @default.
• W1989219210 cites W2019850909 @default.
• W1989219210 cites W2021258781 @default.
• W1989219210 cites W2022231983 @default.
• W1989219210 cites W2022264468 @default.
• W1989219210 cites W2022378387 @default.
• W1989219210 cites W2023495849 @default.
• W1989219210 cites W2024599398 @default.
• W1989219210 cites W2026795906 @default.
• W1989219210 cites W2030866401 @default.
• W1989219210 cites W2032634822 @default.
• W1989219210 cites W2034534661 @default.
• W1989219210 cites W2036113152 @default.
• W1989219210 cites W2038053600 @default.
• W1989219210 cites W2063719206 @default.
• W1989219210 cites W2064076500 @default.
• W1989219210 cites W2068537862 @default.
• W1989219210 cites W2072468474 @default.
• W1989219210 cites W2073143107 @default.
• W1989219210 cites W2073842175 @default.
• W1989219210 cites W2078475344 @default.
• W1989219210 cites W2078797397 @default.
• W1989219210 cites W2079817057 @default.
• W1989219210 cites W2081622755 @default.
• W1989219210 cites W2085179738 @default.
• W1989219210 cites W2085818107 @default.
• W1989219210 cites W2090495550 @default.
• W1989219210 cites W2091701651 @default.
• W1989219210 cites W2094249004 @default.
• W1989219210 cites W2095523961 @default.
• W1989219210 cites W2097597961 @default.
• W1989219210 cites W2109070593 @default.
• W1989219210 cites W2110253451 @default.
• W1989219210 cites W2111817932 @default.
• W1989219210 cites W2116951276 @default.
• W1989219210 cites W2126026910 @default.
• W1989219210 cites W2131757010 @default.
• W1989219210 cites W2134770831 @default.
• W1989219210 cites W2149522724 @default.
• W1989219210 cites W2168563946 @default.
• W1989219210 cites W3099591399 @default.
• W1989219210 cites W3099665156 @default.
• W1989219210 cites W3100434137 @default.
• W1989219210 cites W3103101266 @default.
• W1989219210 cites W3103719627 @default.
• W1989219210 cites W3103761431 @default.
• W1989219210 cites W3122416525 @default.
• W1989219210 cites W4246944130 @default.
• W1989219210 cites W4289924294 @default.
• W1989219210 cites W4297126491 @default.
• W1989219210 cites W4297889187 @default.
• W1989219210 cites W4298080973 @default.
• W1989219210 cites W2072073475 @default.
• W1989219210 doi "https://doi.org/10.1086/376840" @default.
• W1989219210 hasPublicationYear "2003" @default.
• W1989219210 type Work @default.
• W1989219210 sameAs 1989219210 @default.
• W1989219210 citedByCount "180" @default.
• W1989219210 countsByYear W19892192102012 @default.
• W1989219210 countsByYear W19892192102013 @default.
• W1989219210 countsByYear W19892192102014 @default.
• W1989219210 countsByYear W19892192102015 @default.
• W1989219210 countsByYear W19892192102016 @default.
• W1989219210 countsByYear W19892192102017 @default.
• W1989219210 countsByYear W19892192102018 @default.
• W1989219210 countsByYear W19892192102019 @default.
• W1989219210 countsByYear W19892192102020 @default.

• next