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Response to Comment on "An excess of massive stars in the local 30 Doradus starburst".
Schneider, Fabian R N; Sana, Hugues; Evans, Christopher J; Bestenlehner, Joachim M; Castro, Norberto; Fossati, Luca; Gräfener, Götz; Langer, Norbert; Ramírez-Agudelo, Oscar H; Sabín-Sanjulián, Carolina; Simón-Díaz, Sergio; Tramper, Frank; Crowther, Paul A; de Koter, Alexander; de Mink, Selma E; Dufton, Philip L; Garcia, Miriam; Gieles, Mark; Hénault-Brunet, Vincent; Herrero, Artemio; Izzard, Robert G; Kalari, Venu; Lennon, Danny J; Maíz Apellániz, Jesús; Markova, Nevy; Najarro, Francisco; Podsiadlowski, Philipp; Puls, Joachim; Taylor, William D; van Loon, Jacco Th; Vink, Jorick S; Norman, Colin.
Afiliação
  • Schneider FRN; Department of Physics, University of Oxford, Oxford OX1 3RH, UK. fabian.schneider@physics.ox.ac.uk.
  • Sana H; Institute of Astrophysics, KU Leuven, 3001 Leuven, Belgium.
  • Evans CJ; UK Astronomy Technology Centre, Royal Observatory Edinburgh, Edinburgh EH9 3HJ, UK.
  • Bestenlehner JM; Max-Planck-Institut für Astronomie, 69117 Heidelberg, Germany.
  • Castro N; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK.
  • Fossati L; Department of Astronomy, University of Michigan, Ann Arbor, MI 48109, USA.
  • Gräfener G; Austrian Academy of Sciences, Space Research Institute, 8042 Graz, Austria.
  • Langer N; Argelander-Institut für Astronomie der Universität Bonn, 53121 Bonn, Germany.
  • Ramírez-Agudelo OH; Argelander-Institut für Astronomie der Universität Bonn, 53121 Bonn, Germany.
  • Sabín-Sanjulián C; UK Astronomy Technology Centre, Royal Observatory Edinburgh, Edinburgh EH9 3HJ, UK.
  • Simón-Díaz S; Departamento de Física y Astronomía, Universidad de La Serena, La Serena, Chile.
  • Tramper F; Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.
  • Crowther PA; Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain.
  • de Koter A; European Space Astronomy Centre, Mission Operations Division, 28691 Villanueva de la Cañada, Madrid, Spain.
  • de Mink SE; Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK.
  • Dufton PL; Institute of Astrophysics, KU Leuven, 3001 Leuven, Belgium.
  • Garcia M; Astronomical Institute Anton Pannekoek, Amsterdam University, 1098 XH Amsterdam, Netherlands.
  • Gieles M; Astronomical Institute Anton Pannekoek, Amsterdam University, 1098 XH Amsterdam, Netherlands.
  • Hénault-Brunet V; Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, Northern Ireland, UK.
  • Herrero A; Centro de Astrobiología (CSIC-INTA), E-28850 Torrejón de Ardoz, Madrid, Spain.
  • Izzard RG; Department of Physics, Faculty of Engineering and Physical Sciences, University of Surrey, Guildford GU2 7XH, UK.
  • Kalari V; National Research Council, Herzberg Astronomy & Astrophysics, Victoria, BC V9E 2E7, Canada.
  • Lennon DJ; Department of Astrophysics/IMAPP, Radboud University, NL-6500 GL Nijmegen, Netherlands.
  • Maíz Apellániz J; Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.
  • Markova N; Departamento de Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain.
  • Najarro F; Department of Physics, Faculty of Engineering and Physical Sciences, University of Surrey, Guildford GU2 7XH, UK.
  • Podsiadlowski P; Institute of Astronomy, The Observatories, Cambridge CB3 0HA, UK.
  • Puls J; Departamento de Astronomía, Universidad de Chile, Las Condes, Santiago, Casilla 36-D, Chile.
  • Taylor WD; European Space Astronomy Centre, Mission Operations Division, 28691 Villanueva de la Cañada, Madrid, Spain.
  • van Loon JT; Centro de Astrobiología, CSIC-INTA, ESAC Campus, E-28 692 Villanueva de la Cañada, Spain.
  • Vink JS; Institute of Astronomy with National Astronomical Observatory, Bulgarian Academy of Sciences, 4700 Smoljan, Bulgaria.
  • Norman C; Centro de Astrobiología (CSIC-INTA), E-28850 Torrejón de Ardoz, Madrid, Spain.
Science ; 361(6400)2018 07 27.
Article em En | MEDLINE | ID: mdl-30049852
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.
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Meio Ambiente Extraterreno / Astros Celestes Idioma: En Revista: Science Ano de publicação: 2018 Tipo de documento: Article País de afiliação: Reino Unido
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Meio Ambiente Extraterreno / Astros Celestes Idioma: En Revista: Science Ano de publicação: 2018 Tipo de documento: Article País de afiliação: Reino Unido