Discovery of a supercluster in the Zone of Avoidance in Vela. (8th November 2016)

• Record Type: Journal Article
• Authors: Kraan-Korteweg, Renée C.; Cluver, Michelle E.; Bilicki, Maciej; Jarrett, Thomas H.; Colless, Matthew; Elagali, Ahmed; Böhringer, Hans; Chon, Gayoung
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 466:Number 1(2017:Mar.)
• Page Start: L29
• Page End: L33
• Publication Date: 2016-11-08
• Subjects: techniques: spectroscopic -- surveys -- galaxies: clusters: general -- galaxies: distances and redshifts -- cosmology: observations -- large-scale structure of Universe; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slw229
• Languages: English
• ISSNs: 1745-3933

Abstract

Abstract: We report the discovery of a potentially major supercluster that extends across the Galactic plane in the constellation of Vela, at a mean recessional velocity of ∼18 000 km s −1 . Recent multiobject spectroscopic observations of this Vela supercluster (VSCL), using AAOmega+2dF and the Southern African Large Telescope, confirm an extended galaxy overdensity in the Zone of Avoidance (ZOA) located where residual bulk flows predict a considerable mass excess. We present a preliminary analysis of ∼4500 new spectroscopic galaxy redshifts obtained in the ZOA centred on the Vela region ($l = 272{^{\circ}_{.}}5 \pm 20^\circ, b = 0^\circ \pm 10^\circ$ ). The presently sparsely sampled data set traces an overdensity that covers $25^\circ$ in Galactic longitude on either side of the Galactic plane, suggesting an extent of 25 × 20 deg 2, corresponding to ∼ 115 × 90 h 70 Mpc at the supercluster redshift. In redshift space, the overdensity appears to consist of two merging wall-like structures, interspersed with clusters and groups. Both the velocity histogram and the morphology of the multibranching wall structure are consistent with a supercluster classification. $K_{\rm s}^{\rm o}$ galaxy counts show an enhancement of ∼1.2 over the survey area for galaxies brighter than $M_{K}^{\ast }$ at the VSCL distance, and a galaxy overdensity of δ = 0.50–0.77 within a photometric redshift shell around the VSCL, when compared with various Two Micron All-Sky Survey samples. Taking account of selection effects, the VSCL is estimated to contribute $v_\mathrm{LG} \gtrsim 50$ km s −1 to the motion of the Local Group.