Zobrazeno 1 - 10
of 305
pro vyhledávání: '"Lake G"'
Publikováno v:
HIV/AIDS: Research and Palliative Care, Vol Volume 12, Pp 769-778 (2020)
Fikadu Wondimu,1 Fisseha Yetwale,2 Endashew Admassu,2 Wakgari Binu,3 Gizachew Abdissa Bulto,1 Getie Lake,2 Eden Girmaye,1 Kababa Temesgen,1 Taklu Marama4 1Department of Midwifery, College of Medicine and Health Sciences, Ambo University, Ambo, Ethiop
Externí odkaz:
https://doaj.org/article/55e99f4510cc442d936ff6e99afa0484
Publikováno v:
EPJ Web of Conferences, Vol 19, p 01008 (2012)
We study the systematic problems in determining the local dark matter density ρdm(R☉) from kinematics of stars in the Solar Neighbourhood, using a simulated Milky Way-like galaxy. We introduce a new unbiased method for recovering ρdm(R☉) based
Externí odkaz:
https://doaj.org/article/df231d70a43f463e8de15bd1c4c2893b
Publikováno v:
In Evaluation and Program Planning June 2022 92
Metal poor globular clusters (MPGCs) are a unique probe of the early universe, in particular the reionization era. Systems of globular clusters in galaxy clusters are particularly interesting as it is in the progenitors of galaxy clusters that the ea
Externí odkaz:
http://arxiv.org/abs/1403.3953
Tidal streams are a powerful probe of the Milky Way (MW) potential shape. In this paper, we introduce a simple test particle method to fit stream data, using a Markov Chain Monte Carlo technique to marginalise over uncertainties in the progenitor's o
Externí odkaz:
http://arxiv.org/abs/1308.2235
Stellar streams provide unique probes of galactic potentials, with the longer streams normally providing the cleaner measurements. In this paper, we show an example of a short tidal stream that is particularly sensitive to the shape of the Milky Way'
Externí odkaz:
http://arxiv.org/abs/1204.5771
We calculate orbits for the Milky Way dwarf galaxies with proper motions, and compare these to subhalo orbits in a high resolution cosmological simulation. We use the simulation data to assess how well orbits may be recovered in the face of measureme
Externí odkaz:
http://arxiv.org/abs/1001.1731
Publikováno v:
AIP Conf.Proc.1240:415-416,2010
We calculate orbits for the Milky Way dwarf galaxies with proper motions, and compare these to subhalo orbits in a high resolution cosmological simulation. We use this same simulation to assess how well are able to recover orbits in the face of measu
Externí odkaz:
http://arxiv.org/abs/0912.3276
Autor:
Feldmann, R., Carollo, C. M., Mayer, L., Renzini, A., Lake, G., Quinn, T., Stinson, G. S., Yepes, G.
Publikováno v:
Astrophys.J.709:218-240,2010
We trace the evolution of central galaxies in three ~10^13 M_sun galaxy groups simulated at high resolution in cosmological hydrodynamical simulations. The evolution in the group potential leads, at z=0, to central galaxies that are massive, gas-poor
Externí odkaz:
http://arxiv.org/abs/0906.3022
Making robust predictions for the phase space distribution of dark matter at the solar neighbourhood is vital for dark matter direct detection experiments. To date, almost all such predictions have been based on simulations that model the dark matter
Externí odkaz:
http://arxiv.org/abs/0902.0009