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He's a massive star with out-of-this-world charisma.
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Now we compare FUV luminosity (mainly from massive stars) with TIR luminosity (mainly from dust) for the sample galaxies.
A SAGE catalog of massive stars with accurate spectral types and multiwavelengths in the Large Magellanic Cloud includes 1750 objects (Bonanos et al., 2009).
Nearly all types of massive stars with radiatively driven stellar winds are X-ray sources that can be observed by the presently operating powerful X-ray telescopes.
Highly massive stars (with 25 or more times the mass of the Sun) can lose up to 10−5 solar masses each year the equivalent of every 100,000 years.
At this rate, a super-massive star with ({simeq}10^{6}mbox { M}_{odot}) would form after only ({simeq}1mbox { Myr}) (see also Inayoshi and Haiman 2014).
One of these star clusters contains R136a1, the most massive star known, with a mass 265 times that of the Sun.
"When a massive star collides with a low-mass star, the small star gets disrupted to form a disk around the massive one," Livio explains.
The Dutch team postulates in Nature that an older massive star collided with a younger, smaller, hydrogen-rich star, which boosted its hydrogen content.
Supernova remnant Cassiopeia A, as observed 325 years after a massive star exploded, with blue representing X-ray emissions, green representing visible light, and red representing infrared emissions (image by NASA).
Finally, super-massive stars with ({simeq}10^{5}mbox10^{6}mbox { M}_{odot}) may form in atomic cooling halos in which previous star formation was suppressed.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com