Astrophysicist Famaey Benedict is a specialist galaxies and Mond. CNRS researcher, he worked at the observatory in Strasbourg. © Pierre Maraval
And the researcher noted that: "Here also, we show that our findings are at odds with an isotropic distribution to 99.994%, so you could say that by combining with the previous probability, there is one chance in 1.5 billion to observe it in a well-described by simulations under the standard model like the universe Millennium II we have taken as a basis for our work. This is not to say that we must immediately reject this model, but at least these simulations do not account for something really fundamental that escapes us " .
In a previous interview, Benedict Famaey had explained that in the case of dwarf galaxies around the Milky Way, and he seems in the case of those around Andromeda, everything happens as if they contained a lot of dark matter . Enjoy Coloring As tidal dwarfs, they should not, but one can naturally explain these observations with Mond , given the very weak gravitational acceleration inside these small galaxies. Is there a similar problem with the new dwarf galaxies observed?
And the researcher noted that: "Here also, we show that our findings are at odds with an isotropic distribution to 99.994%, so you could say that by combining with the previous probability, there is one chance in 1.5 billion to observe it in a well-described by simulations under the standard model like the universe Millennium II we have taken as a basis for our work. This is not to say that we must immediately reject this model, but at least these simulations do not account for something really fundamental that escapes us " .
In a previous interview, Benedict Famaey had explained that in the case of dwarf galaxies around the Milky Way, and he seems in the case of those around Andromeda, everything happens as if they contained a lot of dark matter . Enjoy Coloring As tidal dwarfs, they should not, but one can naturally explain these observations with Mond , given the very weak gravitational acceleration inside these small galaxies. Is there a similar problem with the new dwarf galaxies observed?