An excess of massive stars in the local 30 Doradus starburst

@article{Schneider2018AnEO,
  title={An excess of massive stars in the local 30 Doradus starburst},
  author={Fabian R. N. Schneider and Hugues Sana and C. J. Evans and Joachim M. Bestenlehner and Norberto Castro and Luca Fossati and G{\"o}tz Gr{\"a}fener and Norbert Langer and Oscar Hern{\'a}n Ram{\'i}rez-Agudelo and Carolina Sab{\'i}n-Sanjuli{\'a}n and Sergio Sim{\'o}n-D{\'i}az and Frank Tramper and Paul A. Crowther and Alexander de Koter and Selma E. de Mink and Philip L. Dufton and M. Garcia and Mark Gieles and Vincent H{\'e}nault-Brunet and A. Herrero and Robert G. Izzard and Venu M. Kalari and Daniel J. Lennon and Jes{\'u}s Ma{\'i}z Apell{\'a}niz and N. Markova and Francisco Najarro and Philipp Podsiadlowski and Joachim Puls and William D. Taylor and Jacco Th. van Loon and Jorick S. Vink and Colin Norman},
  journal={Science},
  year={2018},
  volume={359},
  pages={69 - 71}
}
Observing more massive stars The number of stars that form at each mass is known as the initial mass function (IMF). For most masses, the IMF follows a power-law distribution, first determined by Edwin Salpeter in 1955. Schneider et al. used observations of the nearby star-forming region 30 Doradus (also known as the Tarantula Nebula) and combined these with stellar modeling to determine its IMF. They found more stars above 30 solar masses than predicted by the Salpeter distribution. Because… 
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