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pro vyhledávání: '"Elliot Y Davies"'
Autor:
Vasily Belokurov, Eugene Vasiliev, Alis J Deason, Sergey E Koposov, Azadeh Fattahi, Adam M Dillamore, Elliot Y Davies, Robert J J Grand
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023, Vol.518(4), pp.6200-6215 [Peer Reviewed Journal]
Belokurov, V, Vasiliev, E, Deason, A J, Koposov, S E, Fattahi, A, Dillamore, A M, Davies, E Y & Grand, R J J 2023, ' Energy wrinkles and phase-space folds of the last major merger ', Monthly Notices of the Royal Astronomical Society, vol. 518, no. 4, pp. 6200-6215 . https://doi.org/10.1093/mnras/stac3436
Belokurov, V, Vasiliev, E, Deason, A J, Koposov, S E, Fattahi, A, Dillamore, A M, Davies, E Y & Grand, R J J 2023, ' Energy wrinkles and phase-space folds of the last major merger ', Monthly Notices of the Royal Astronomical Society, vol. 518, no. 4, pp. 6200-6215 . https://doi.org/10.1093/mnras/stac3436
Relying on the dramatic increase in the number of stars with full 6D phase-space information provided by the Gaia Data Release 3, we discover unambiguous signatures of phase-mixing in the stellar halo around the Sun. We show that for the stars likely
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::293b526458db8422226e6f1f92871d63
https://doi.org/10.1093/mnras/stac3436
https://doi.org/10.1093/mnras/stac3436
In a galaxy merger, the stars tidally stripped from the satellite and accreted onto the host galaxy undergo phase mixing and form finely-grained structures in the phase space. However, these fragile structures may be destroyed in the subsequent galax
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78c932763367dbfe06863776b86677e2
Recent work uncovered features in the phase space of the Milky Way's stellar halo which may be attributed to the last major merger. When stellar material from a satellite is accreted onto its host, it phase mixes and appears finely substructured in p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8c13ccadbbfada5e3225c938ef0e3ee
http://arxiv.org/abs/2210.05679
http://arxiv.org/abs/2210.05679
Publikováno v:
Journal of Cosmology and Astroparticle Physics
We present numerical relativity simulations of cosmological scenarios in which the universe is smoothed and flattened by undergoing a phase of slow contraction and test their sensitivity to a wide range of initial conditions. Our numerical scheme ena
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::986ee8a2637a31bd7770ee7e458ae3ba
https://hdl.handle.net/21.11116/0000-0006-C627-F21.11116/0000-0006-C629-D21.11116/0000-0007-0FDD-1
https://hdl.handle.net/21.11116/0000-0006-C627-F21.11116/0000-0006-C629-D21.11116/0000-0007-0FDD-1