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Theoretical limit of star size (Large Magellanic Cloud) ≳1,550 [9] L/T eff: Estimated by measuring the fraction of red supergiants at higher luminosities in a large sample of stars. Assumes an effective temperature of 3545 K. Reported for reference: HV 888 1,477 [102] –1,584 [103] Large Magellanic Cloud L/T eff: HD 269551 A 1,439 [104 ...
Some stars may once have been more massive than they are today. It is likely that many large stars have suffered significant mass loss (perhaps as much as several tens of solar masses). This mass may have been expelled by superwinds: high velocity winds that are driven by the hot photosphere into interstellar space. The process forms an ...
A giant star has a substantially larger radius and luminosity than a main-sequence (or dwarf) star of the same surface temperature. [1] They lie above the main sequence (luminosity class V in the Yerkes spectral classification) on the Hertzsprung–Russell diagram and correspond to luminosity classes II and III. [2]
Print/export Download as PDF; ... It is the central star of Hen 2-131 Planetary Nebula. Cygnus X-1: ... The Large Magellanic Cloud ...
S Doradus (also known as S Dor) is one of the brightest stars in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, located roughly 160,000 light-years away. The star is a luminous blue variable , and one of the most luminous stars known , having a luminosity varying widely above and below 1,000,000 times the luminosity of ...
A star is a massive luminous spheroid astronomical object made of plasma that is held together by its own gravity.Stars exhibit great diversity in their properties (such as mass, volume, velocity, stage in stellar evolution, and distance from Earth) and some of the outliers are so disproportionate in comparison with the general population that they are considered extreme.
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This is a binary star system with an orbital period of 84.1 days. [ 14 ] [ 15 ] The primary component is a B1 giant or subgiant star. [ 3 ] This is a large star with nearly eleven [ 8 ] times the mass and over six times the radius of the Sun. [ 9 ] Pi Aquarii shines about 7,300 [ 10 ] times as brightly as the Sun.
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