The impact of massive stars and black holes on the fate of open star clusters and their tidal streams

@article{Wang2021TheIO,
  title={The impact of massive stars and black holes on the fate of open star clusters and their tidal streams},
  author={Long Wang and Tereza Jerabkova Department of Astronomy and School of Materials Science and The University of Tokyo and 7-3-1 Hongo and Bunkyo-ku and Tokyo and 113-0033 and Japan. and Riken Center for Computational Science and 7-1-26 Minatojima-minami-machi and Chuo-ku and Kobe and Hyogo 648-0047 and European Space Agency and European Space Research and Technology Centre and 1 Keplerlaan and 2201 AZ Noordwijk and The Netherlands.},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Context. To investigate how the content of massive OB stars affects the long-term evolution of young open clusters and their tidal streams, and how such an effect influences the constraint of initial conditions by looking at the present-day observations. Aims. OB stars are typically in binaries, have a strong wind mass loss during the first few Myr, and many become black holes. These affect the dynamical evolution of an open star cluster and impact its dissolution in a given Galactic potential… Expand

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