Just spotted this, great image.
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That is Awsome i didnt even see all the other ones how big would that new star R136a1 be on that scale
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Crowther's paper gives a radius of ~35 times that of the sun, so it's actually rather small in these terms.
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Always sets me wondering what these stars do look like close-up.
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The largest stars probably aren't spherical - both red supergiants and yellow hypergiants look to be non-radial pulsators (see
Astronomy at Vienna University » Research for example) and have very low surface gravities so are barely holding themselves together against radiation pressure. They're also losing mass at huge rates, as much as a solar mass every thousand to ten-thousand years, to the extent that the wind is opaque at at least some wavelengths and it's somewhat debatable where the edge of the star is - if you measure stellar radii with interferometry you get different answers depending on the wavelength you pick.
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