2010/01/31 by Maciej Bilicki, Michał Chodorowski, Michał J. Chodorowski
Physics and Astronomy · #Amplitude #Astronomy and Astrophysical Research #Cosmic microwave background #Density contrast #Dipole #Galaxies: Formation, Evolution, Phenomena #Galaxy #Local Void #Radio Astronomy Observations and Technology #Spurious relationship #Void (composites) #astro-ph.CO
paper · pdf · doi:10.1111/j.1365-2966.2010.16771.x
published as Monthly Notices of the Royal Astronomical Society, 2010, Volume 406 Issue 2, Pages 1358 - 1363 · 6 pages, 2 figures; revised version, slightly expanded, accepted for publication in MNRAS.
arxiv created 2010/03/31 · openalex publication_date 2010/05/01 · arxiv updated 2010/07/21 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
In measurements of the clustering dipole from all-sky surveys, an important problem is the lack of information about galaxy distribution in the so-called zone of avoidance (ZoA). The existence of the Local Void (LV) has a systematic effect on these measurements. If the ZoA is randomly filled with mock galaxies, then the calculated acceleration of the Local Group (LG) of galaxies has a spurious component, resulting from the lack of real galaxies in the intersection of the LV with the ZoA. This component affects both the misalignment angle between the clustering dipole and the CMB dipole, and the inferred value of mean matter density Ωm. We calculate the amplitude of the spurious acceleration acting on the LG due to the LV. Its value depends on the geometry and size of the LV, as well as on its density contrast. However, under the simplest assumption of the LV being spherical and completely empty, within the linear theory this amplitude amounts only to about 45 km s−1 in units of velocity. The resulting change in the misalignment angle is smaller than 1°, and the fractional change in the deduced value of Ωm is about 5 per cent. Accounting for observationally indicated elongation of the LV and maintaining the maximizing assumption of a complete lack of galaxies inside increases these numbers only moderately. Specifically, the amplitude of the spurious acceleration rises to about 60 km s−1, the misalignment angle remains still smaller than 1° and the fractional change in the deduced value of Ωm is enhanced to about 7 per cent. Thus, despite the overall importance of the LV for the motion of the LG, the influence of the intersection of the LV with the ZoA on measurements of the clustering dipole is found to be only a minor systematic effect.