The coherent motion of Cen A dwarf satellite galaxies remains a challenge for ΛCDM cosmology
The coherent motion of Cen A dwarf satellite galaxies remains a challenge for ΛCDM cosmology
复制标题
Cen A矮卫星星系的相干运动仍然是ΛCDM宇宙学的挑战
DOI:
10.1051/0004-6361/202039973
复制
发表时间:
2020
影响因子:
6.5
通讯作者:
H. Jerjen
中科院分区:
文献类型:
--
作者:
O. Muller;M. Pawlowski;F. Lelli;K. Fahrion;M. Rejkuba;M. Hilker;Jamie Kanehisa;N. Libeskind;H. Jerjen
The plane-of-satellites problem is one of the most severe small-scale challenges for the standard Λ cold dark matter (ΛCDM) cosmological model: Several dwarf galaxies around the Milky Way and Andromeda co-orbit in thin, planar structures. A similar case has been identified around the nearby elliptical galaxy Centaurus A (Cen A). In this Letter, we study the satellite system of Cen A, adding twelve new galaxies with line-of-sight velocities from VLT/MUSE observations. We find that 21 out of 28 dwarf galaxies with measured velocities share a coherent motion. Similarly, flattened and coherently moving structures are found only in 0.2% of Cen A analogs in the Illustris-TNG100 cosmological simulation, independently of whether we use its dark-matter-only or hydrodynamical run. These analogs are not co-orbiting, and they arise only by chance projection, thus they are short-lived structures in such simulations. Our findings indicate that the observed co-rotating planes of satellites are a persistent challenge for ΛCDM, which is largely independent from baryon physics.
影响因子:
4.8
作者:
J. Samuel;A. Wetzel;S. Chapman;E. Tollerud;P. Hopkins;M. Boylan-Kolchin;J. Bailin;C. Faucher-Giguère
通讯作者:
J. Samuel;A. Wetzel;S. Chapman;E. Tollerud;P. Hopkins;M. Boylan-Kolchin;J. Bailin;C. Faucher-Giguère