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Gaia + PeTar projects combines N-body simulations with Gaia eDR3 data to robustly identify tidal tails of open star clusters in the Milky Way disc. As a first results, Jerabkova et al. (A&A, 2021) presents a detection of the full extent (1kpc!) of tidal tail of the Hyades star cluster and the first even detection of substructures in the tail of open star cluster putting constraints on the MW potential. Follow up studies are coming up, see Long & Jerabkova (A&A, 2021). Tidal Tails tell us the tale of cluster formation and evolution and of the Milky Way potential that has impacted the stars and our Gaia + PeTar project is taking full advantage of that.
star cluster, tidal tails, Nbody simulations, Gaia, Galactic disk, Galactic potential
star cluster, tidal tails, Nbody simulations, Gaia, Galactic disk, Galactic potential
citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
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