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Response to Comment on “An excess of massive stars in the local 30 Doradus starburst”

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.
Publication status:
Published
Peer review status:
Reviewed (other)
Version:
Accepted Manuscript

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Publisher copy:
10.1126/science.aat7032

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Astrophysics
ORCID:
0000-0002-5965-1022
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ORCID:
0000-0001-6656-4130
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ORCID:
0000-0002-0859-5139
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ORCID:
0000-0003-0521-473X
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Oxford Hintze Centre for Astrophysical Surveys More from this funder
Publisher:
American Association for the Advancement of Science Publisher's website
Journal:
Science Journal website
Volume:
361
Issue:
6400
Pages:
Article: eaat7032
Publication date:
2018-07-27
Acceptance date:
2018-06-04
DOI:
EISSN:
1095-9203
ISSN:
0036-8075
Pubs id:
pubs:891621
URN:
uri:855b1f27-ad0e-4ac6-9b61-60130f124884
UUID:
uuid:855b1f27-ad0e-4ac6-9b61-60130f124884
Local pid:
pubs:891621

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