1 code implementation • 11 Mar 2013 • Jaime E. Forero-Romero, Yehuda Hoffman, Sebastian Bustamante, Stefan Gottloeber, Gustavo Yepes
It follows that within current observational uncertainties the quasi-conserved quantities that characterize the orbit of the LG, i. e. e_tot, r_orb and lambda, do not challenge the standard LCDM model, but the model is in tension with regard to the actual values of the radial and tangential velocities.
Cosmology and Nongalactic Astrophysics
