中文
相关论文

相关论文: Messier 81's Planck view vs its halo mapping

200 篇论文

In several spiral galaxies that are observed face-on, large-scale ordered magnetic fields (the so-called magnetic arms) were found. One of the explanations was the action of the magnetic reconnection, which leads to a higher ordering of the…

星系天体物理 · 物理学 2022-09-14 M. Wezgowiec , R. Beck , M. Hanasz , M. Soida , M. Ehle , R. -J. Dettmar , M. Urbanik

We search for an unusual alignment of the preferred axes of the quadrupole and octopole, the so-called axis of evil, in the CMB temperature and polarization data from WMAP. We use the part of the polarization map which is uncorrelated with…

宇宙学与河外天体物理 · 物理学 2010-03-22 Mona Frommert , Torsten A. Ensslin

We present a theoretical study of CMB temperature peaks, including its effect over the polarization field, and allowing nonzero eccentricity. The formalism is developed in harmonic space and using the covariant derivative on the sphere,…

宇宙学与河外天体物理 · 物理学 2016-05-25 A. Marcos-Caballero , R. Fernández-Cobos , E. Martínez-González , P. Vielva

In this paper, we review the approach leading to cosmic polarization rotation observation and present the current status with an outlook. In the study of the relations among equivalence principles, we found that long-range…

天体物理学 · 物理学 2009-06-23 Wei-Tou Ni

Recent papers have reported an unexplained cooling of CMB photons passing through galaxies in nearby cosmic filaments $z<0.02$ at the $>5\sigma$ level. Here we show for the first time that this effect is also present at higher redshifts…

宇宙学与河外天体物理 · 物理学 2026-04-20 Juan Ignacio Domínguez Feldman , Luis A. Pereyra , Frode K. Hansen , Facundo Toscano , Diego Garcia Lambas

Scattering of cosmic microwave background (CMB) radiation in galaxy clusters induces polarization signals determined by the quadrupole anisotropy in the photon distribution at the location of clusters. This "remote quadrupole" derived from…

宇宙学与河外天体物理 · 物理学 2016-07-13 Guo-Chin Liu , Kiyotomo Ichiki , Hiroyuki Tashiro , Naoshi Sugiyama

The peculiar motion of an observer with respect to the CMB rest frame induces a deflection in the arrival direction of the observed photons (also known as CMB aberration) and a Doppler shift in the measured photon frequencies. As a…

宇宙学与河外天体物理 · 物理学 2015-06-12 Riccardo Catena , Michele Liguori , Alessio Notari , Alessandro Renzi

Inspired by a dipole asymmetric template for the CMB temperature map in the primordial scalar fluctuations observed by Planck at a large scale, we examine the contribution of a similar template for power asymmetry in modifying the linear…

广义相对论与量子宇宙学 · 物理学 2023-08-01 Jafar Khodagholizadeh , Rohoollah Mohammadi , S. M. S. Movahed

An observer in relative motion to the Cosmic Microwave Background (CMB) rest frame is sensitive to both aberration and Doppler effects. Both effects introduce similar but non-identical off-diagonal couplings in the spherical harmonic…

宇宙学与河外天体物理 · 物理学 2021-09-06 Pedro da Silveira Ferreira , Miguel Quartin

Measurements of intensity and polarization of diffuse Galactic synchrotron emission as well as starlight polarization reveal power law spectra of fluctuations. We show that these fluctuations can arise from magnetohydrodynamic (MHD)…

天体物理学 · 物理学 2016-08-30 Jungyeon Cho , A. Lazarian

The halo mass-temperature relation for a sample of 216 galaxy clusters, groups, and individual galaxies observed by $Chandra$ X-ray Observatory is presented. Using accurate spectral measurements of their hot atmospheres, we derive the $M-T$…

星系天体物理 · 物理学 2023-04-06 Iurii Babyk , Brian McNamara

The recent Planck results and future releases on the horizon present a key opportunity to address a fundamental question in inflationary cosmology of whether primordial density perturbations have a quantum or thermal origin, i.e. whether…

宇宙学与河外天体物理 · 物理学 2013-06-20 Sam Bartrum , Arjun Berera , Joao G. Rosa

This paper presents 12CO J=3-2, 13CO J=3-2, C18O J=3-2, and 13CO J=2-1 spectra of the irregular starburst galaxy M82 taken with the 15 m James Clerk Maxwell Telescope. All maps exhibit a double peaked morphology, despite evidence that the…

天体物理学 · 物理学 2009-10-31 Glen R. Petitpas , Christine D. Wilson

Spatially fluctuating primordial magnetic fields (PMFs) inhomogeneously reheat the Universe when they dissipate deep inside the horizon before recombination. Such an energy injection turns into an additional photon temperature perturbation.…

宇宙学与河外天体物理 · 物理学 2019-11-28 Shohei Saga , Atsuhisa Ota , Hiroyuki Tashiro , Shuichiro Yokoyama

Part of the CMB polarization signal in the direction of galaxy clusters is produced by Thomson scattering of the CMB temperature quadrupole. In principle this allows measurement of the CMB power spectrum harmonic $C_2(z)$ with higher…

天体物理学 · 物理学 2009-09-29 Jamie Portsmouth

The recent observations from the James Webb Space Telescope have led to a surprising discovery of a significant density of massive galaxies with masses of $M \ge 10^{10.5} M_{\odot}$ at redshifts of approximately $z\sim 10$. This…

宇宙学与河外天体物理 · 物理学 2023-10-10 Matteo Forconi , Ruchika , Alessandro Melchiorri , Olga Mena , Nicola Menci

The Cold Spot, with an unusually cold region surrounded by a hot ring, is a statistically significant anomaly in the Cosmic Microwave Background (CMB) sky. In this work we assess whether different sets of multiple subvoids based on the…

宇宙学与河外天体物理 · 物理学 2021-01-13 Marzieh Farhang , M. Sadegh Movahed

NGC 891 is a nearby edge-on galaxy that is similar to the Milky Way and has a hot X-ray emitting halo that could arise from accretion, a galactic fountain, or a combination of the two. The metallicity of the gas can help distinguish between…

宇宙学与河外天体物理 · 物理学 2015-06-12 Edmund J. Hodges-Kluck , Joel N. Bregman

Weak lensing effects are known to introduce non-linear couplings in CMB temperature maps. In inflationary scenario, the primary CMB anisotropies are expected to form a 2D Gaussian map, for which, the probability distribution function of the…

天体物理学 · 物理学 2011-05-23 F. Bernardeau

We study the Planck CMB temperature at different scales through its derivatives up to second order, which allows one to characterize the local shape and isotropy of the field. The problem of having an incomplete sky in the calculation and…

宇宙学与河外天体物理 · 物理学 2017-02-22 A. Marcos-Caballero , E. Martínez-González , P. Vielva