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Science ; 361(6400)2018 07 27.
Artículo en Inglés | MEDLINE | ID: mdl-30049852

RESUMEN

Farr and Mandel reanalyze our data, finding initial mass function slopes for high-mass stars in 30 Doradus that agree with our results. However, their reanalysis appears to underpredict the observed number of massive stars. Their technique results in more precise slopes than in our work, strengthening our conclusion that there is an excess of massive stars (>30 solar masses) in 30 Doradus.


Asunto(s)
Medio Ambiente Extraterrestre , Estrellas Celestiales , Tiempo
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