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The bright component of the binary is a blue-white star 24.7 times as luminous as the Sun.
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AutoDensity is not limited to specific machine brands and models of analogue mammogram machines because it flexibly identifies and removes the range of background artefacts generated by different film cassettes, and it replicates the Cumulus reader-driven approach of classifying as dense tissue the relatively bright components of the breast image.
It is a binary star, the brighter component of which is an orange giant and the fainter a yellow-white main sequence star.
Cor Caroli, also called Alpha Canum Venaticorum, binary star located 110 light-years from Earth in the constellation Canes Venatici and consisting of a brighter component (A) of visual magnitude 2.9 and a companion (B) of magnitude 5.5.
The dark component is probably due to the infall of carbonaceous material, whereas the bright component is the original Vesta basaltic soil.
The second brightest component, Alpha Centauri B, of visual magnitude 1.4, is a redder star.
A shallower secondary eclipse occurs when the brighter component passes in front of the other; it corresponds to an annular eclipse (or transit).
The brighter component is a bluish Be star of spectral type B5IV+ and magnitude 4.51, while the dimmer component is a yellow star of magnitude 5.5.
The brightest component is a blue-white main sequence star of spectral type B8V, which is 3.5 times as massive and 180 times as luminous as the Sun.
The brighter component, termed Sirius A, is a main-sequence star of spectral type A1V, with an estimated surface temperature of 9,940 K.
The brighter component is a Rapidly oscillating Ap star, pulsating with a period of 16.2 minutes.
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