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
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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
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发表时间:
2020
影响因子:
6.5
通讯作者:
H. Jerjen
H. Jerjen
中科院分区:
物理与天体物理2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

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卫星平面问题是标准Λ冷暗物质(ΛCDM)宇宙学模型最严重的小尺度挑战之一:银河系和仙女座周围的几个矮星系以薄的平面结构共轨。在附近的椭圆星系半人马座A(Cen A)周围也发现了类似的情况。在这封信中,我们研究了Cen A的卫星系统,从VLT/MUSE观测中增加了12个新的星系。我们发现,21的28个矮星系的速度测量共享一个相干运动。同样,在Illustris-TNG 100宇宙学模拟中,只有0.2%的Cen A类似物中发现了扁平和相干移动的结构,这与我们是否使用其仅暗物质或流体动力学运行无关。这些类似物不是共轨的,它们只是通过偶然的投射而出现,因此它们在这种模拟中是短暂的结构。我们的研究结果表明,观测到的卫星同向旋转平面是对ΛCDM的持续挑战,这在很大程度上独立于重子物理。
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.
DOI: 10.1093/mnras/stab955
发表时间: 2020-10
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