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要旨:
Nowadays, publications in astrophysics are mainly published and read in digitized formats. Astrophysical publications in both research and in popular outreach often use colorful representations of stars to indicate various stellar types, that is, different spectral types or effective temperatures. Computer‐generated and computer‐displayed imagery has become an integral part of stellar astrophysics communication. There is, however, no astrophysically motivated standard color palette for illustrative representations of stars, and some stars are actually represented in misleading colors. We use precomputed PHOENIX and TLUSTY stellar model spectra and convolve them with the three standard color‐matching functions for human color perception between 360 and 830 nm. The color‐matching functions represent the three sets of receptors in the eye that respond to red, green, and blue light. For a grid of main‐sequence stars with effective temperatures between 2,300 and 55,000 K of different metallicities, we present the red–blue–green and hexadecimal color codes that can be used for digitized color representations of stars as if seen from space. We find significant deviations between the color codes of stars computed from stellar spectra and from a black body radiator of the same effective temperature. We illustrate the main sequence in the color wheel and demonstrate that there are no yellow, green, cyan, or purple stars. Red dwarf stars (spectral types M0V–M9V) actually look orange to the human eye. Old white dwarfs such as WD 1856 + 534, host to a newly discovered transiting giant planet candidate, appear pale orange to the human eye, not white. Our freely available software can be used to generate color codes for any input spectrum such as those from planets, galaxies, quasars, etc.
