4.7 Article

Fast galaxy bars continue to challenge standard cosmology

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stab2553

关键词

gravitation; instabilities; galaxies: evolution; galaxies: bar; galaxies: spiral

资金

  1. University of Bonn
  2. Alexander von Humboldt Foundation
  3. Agence Nationale de la Recherche [ANR-18-CE31-0006, ANR-19CE31-0017]
  4. European Research Council (ERC) under the European Union [834148]
  5. European Southern Observatory-Government of Chile Joint Committee programme [ORP060/19]
  6. Gauss Centre for Supercomputing (GCS)
  7. European Research Council (ERC) [834148] Funding Source: European Research Council (ERC)

向作者/读者索取更多资源

The study reveals significant discrepancies between cosmological simulations and observations in the evolution of barred galaxies, particularly in the ratio of corotation radius to bar length. The statistical tension in EAGLE50 is lower due to a small number of galaxies suitable for analysis. The simulated fraction of barred galaxies and their trend with stellar mass differ greatly from observations.
Many observed disc galaxies harbour a central bar. In the standard cosmological paradigm, galactic bars should be slowed down by dynamical friction from the dark matter halo. This friction depends on the galaxy's physical properties in a complex way, making it impossible to formulate analytically. Fortunately, cosmological hydrodynamical simulations provide an excellent statistical population of galaxies, letting us quantify how simulated galactic bars evolve within dark matter haloes. We measure bar strengths, lengths, and pattern speeds in barred galaxies in state-of-the-art cosmological hydrodynamical simulations of the IllustrisTNG and EAGLE projects, using techniques similar to those used observationally. We then compare our results with the largest available observational sample at redshift z = 0. We show that the tension between these simulations and observations in the ratio of corotation radius to bar length is 12.62 sigma (TNG50), 13.56 sigma (TNG100), 2.94 sigma (EAGLE50), and 9.69 sigma (EAGLE100), revealing for the first time that the significant tension reported previously persists in the recently released TNG50. The lower statistical tension in EAGLE50 is actually caused by it only having five galaxies suitable for our analysis, but all four simulations give similar statistics for the bar pattern speed distribution. In addition, the fraction of disc galaxies with bars is similar between TNG50 and ING100, though somewhat above EAGLE100. The simulated bar fraction and its trend with stellar mass both differ greatly from observations. These dramatic disagreements cast serious doubt on whether galaxies actually have massive cold dark matter haloes, with their associated dynamical friction acting on galactic bars.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据