Next, you need to do one of the following:ġ) Copy NKFlare.inc and all of the FLR file(s) to your povray "include"Ģ) Copy NKFlare.inc and all of the FLR file(s) to the same directoryģ) Add the directory that contains NKFlare.inc and all of the FLRįiles to your library path. Marble phase (.55) turbulence 0.8 frequency 1.3 povray 3.7 A-type white main sequence star Retrieved November 13, 2021.English: White main sequence star. The Largest Star in the Universe – Size Comparison. Monthly Notices of the Royal Astronomical Society. "The magnetic early B-type Stars II: Stellar atmospheric parameters in the era of Gaia". "Massive pulsating stars observed by BRITE-Constellation. "XMM-Newton observations of β Centauri (B1 III): The temperature structure in the hot plasma and the photosphere-wind connection". "Validation of the new Hipparcos reduction". "Interferometry and spectroscopy of β Cen: a β Cephei star in a binary system". ![]() "A Spectroscopic Study of Two Southern B-Type Variables". CDS/ADC Collection of Electronic Catalogues. "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". New Haven, Conn.: Yale University Observatory, 5th Rev.ed. All stars are blue and in their main-sequence stages. They are shining 25,000 times more powerful than the Sun. Aa and Ab are 10 times more massive than our Sun and 13 times the size.
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