II/19               Colors of F and G dwarfs                     (Bell, 1971)

Theoretical Colours for F and G dwarfs Bell R.A. <Monthly Notices Roy. Astron. Soc 154, 343 (1971)> =1971MNRAS.154..343B 1971MNRAS.154..343B
ADC_Keywords: Colors ; Stars, F-type ; Stars, dwarfs Abstract: Synthetic spectra have been computed for F and G dwarf stars, using a number of values of chemical abundances, Doppler broadening velocity and damping constants. Filter transmission function have been convolved with thee spectra to yield color indices in 3 photometric systems. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 177 58 Theoretical colors for F and G dwarf stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- Seq [1/58] Model sequential number 4- 6 F3.1 --- t0 Boundary reciprocal temperature θ0=T/5040 8- 12 I5 cm/s2 g Gravity 14- 16 F3.1 km/s v Doppler broadening velocity 18- 23 F6.4 --- a Damping constant 25- 28 F4.2 Sun M/H Metal-to-Hydrogen ratio, relative to Sun (2) 30- 33 I4 K Teff Effective temperature 35- 40 F6.3 mag U-B Johnson (U-B) color 42- 47 F6.3 mag B-V Johnson (B-V) color 49- 54 F6.3 mag d(U-B) Contribution of line blocking Δ(U-B) (1) 56- 61 F6.3 mag d(B-V) Contribution of line blocking Δ(B-V) (1) 65- 70 F6.3 mag u-v Stroemgren color (u-v) 72- 77 F6.3 mag v-b Stroemgren color (v-B) 79- 84 F6.3 mag b-y Stroemgren color (b-y) 86- 91 F6.3 mag c1 Stroemgren color c1=(u-v)-(v-b) 93- 98 F6.3 mag m1 Stroemgren color m1=(v-b)-(b-y) 100-105 F6.3 mag u-b Stroemgren color (u-b) 107-112 F6.3 mag d(u-v) Contribution of line blocking Δ(u-v) (1) 114-119 F6.3 mag d(v-b) Contribution of line blocking Δ(v-b) (1) 121-126 F6.3 mag d(b-y) Contribution of line blocking Δ(b-y) (1) 130-135 F6.3 mag 33-52 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color 137-142 F6.3 mag 35-52 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color 144-149 F6.3 mag 37-52 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color 151-156 F6.3 mag 40-52 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color 158-163 F6.3 mag 45-52 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color 165-170 F6.3 mag 52-58 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color 172-177 F6.3 mag 52-63 Johnson (1967CoLPL...6...85J 1967CoLPL...6...85J) color -------------------------------------------------------------------------------- Note (1): the continuum colors are c-Δc, e.g. (U-B)-Δ(U-B) or (B-V)-Δ(B-V) Note (2): the proportion of the elements are, on the logarithmic scale H=12: He=10.80; C=8.62; N=7.88; O=8.86; Mg=7.10; Sc=3.20; Ti=4.58; V=3.97; Ca=6.19; Cr=5.18; Mn=4.95; Fe=6.62; Co=4.77; Ni=5.09; Ce=1.95 -------------------------------------------------------------------------------- Histor The catalogue was prepared at CDS before 1976.
(End) Francois Ochsenbein [CDS] 22-Jul-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line