Published in
American Association for the Advancement of Science, Science, 6400(361), p. eaat7032, 2018
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Response to Comment on “An excess of massive stars in the local 30 Doradus starburst”
Journal article published in 2018 by
Fabian R. N. Schneider 
,
Hugues Sana ,
Christopher J. Evans,
Joachim M. Bestenlehner ,
Norberto Castro ,
Luca Fossati ,
Götz Gräfener ,
Norbert Langer,
Oscar H. Ramírez-Agudelo ,
Carolina Sabín-Sanjulián ,
Sergio Simón-Díaz ,
Frank Tramper ,
Paul A. Crowther ,
Alexander de Koter ,
Selma E. de Mink
and other authors.
,
Hugues Sana ,
Christopher J. Evans,
Joachim M. Bestenlehner ,
Norberto Castro ,
Luca Fossati ,
Götz Gräfener ,
Norbert Langer,
Oscar H. Ramírez-Agudelo ,
Carolina Sabín-Sanjulián ,
Sergio Simón-Díaz ,
Frank Tramper ,
Paul A. Crowther ,
Alexander de Koter ,
Selma E. de Mink
and other authors.
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
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.
