- 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
- Files:
-
-
(pdf, 285.4kb)
-
- Publisher copy:
- 10.1126/science.aat7032
-
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- 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
- Language:
- English
- Keywords:
- Copyright holder:
- American Association for the Advancement of Science
- Copyright date:
- 2018
- Notes:
-
Copyright © 2018, American Association for the Advancement of Science. This is the accepted manuscript version of the article. The final version is available online from the American Association for the Advancement of Science at: https://doi.org/10.1126/science.aat7032
Journal article
Response to Comment on “An excess of massive stars in the local 30 Doradus starburst”
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Oxford Hintze Centre for
Astrophysical Surveys
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