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S Apodis (HD 133444) is an R Coronae Borealis variable star located in the far southern constellation Apus. [1]

5 relations: Apus, Durchmusterung, Henry Draper Catalogue, Luminosity, R Coronae Borealis variable.

Apus is a faint constellation in the southern sky, first defined in the late 16th century.

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In astronomy, Durchmusterung or Bonner Durchmusterung (BD), is the comprehensive astrometric star catalogue of the whole sky, compiled by the Bonn Observatory (Germany) from 1859 to 1903.

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The Henry Draper Catalogue (HD) is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension (HDE), published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the Henry Draper Extension Charts (HDEC), published from 1937 to 1949 in the form of charts, which gave classifications for 86,933 more stars.

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In astronomy, luminosity is the total amount of energy emitted by a star, galaxy, or other astronomical object per unit time.

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An R Coronae Borealis variable (abbreviated RCB, RCrB) is an eruptive variable star that varies in luminosity in two modes, one low amplitude pulsation (a few tenths of a magnitude), and one irregular unpredictably sudden fading by 1 to 9 magnitudes.

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[1] https://en.wikipedia.org/wiki/S_Apodis

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