Tidal tails of star clusters

By A. Küpper, Pavel Kroupa, H. Baumgardt, Douglas Heggie. 2009

135 citations recorded by the source corpus.

Based on recent findings of a formation mechanism of substructure in tidal tails by Kupper et al., we investigate a more comprehensive set of N-body models of star clusters on orbits about a Milky Way like potential. We find that the predicted epicyclic overdensities arise in any tidal tail no matter which orbit the cluster follows as long as the cluster lives long enough for the overdensities to build up.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/2671d81b7abdf4dd6721328140e17801cdae99a2

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In Astronomy and Astrophysics

  1. Hans-Walter Rix
  2. P. Hopkins
  3. L. Hernquist
  4. Pavel Kroupa
  5. Sergey E. Koposov
  6. V. Belokurov
  7. C. Conroy
  8. N. Evans II

In Instrumentation

  1. Hans-Walter Rix
  2. Sergey E. Koposov
  3. David W. Hogg
  4. V. Belokurov
  5. M. Pawlowski
  6. Jo Bovy
  7. Pavel Kroupa
  8. J. Pflamm-Altenburg

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