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arXiv · 1011.5985

On the kinematics of the Local cosmic void

Olga Nasonova·Igor Karachentsev
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Abstract

We collected the existing data on the distances and radial velocities of galaxies around the Local Void in the Aquila/Hercules to examine the peculiar velocity field induced by its underdensity. A sample of 1056 galaxies with distances measured from the Tip of the Red Giant Branch, the Cepheid luminosity, the SNIa luminosity, the surface brightness fluctuation method, and the Tully-Fisher relation has been used for this purpose. The amplitude of outflow is found to be ~300 km/s. The galaxies located within the void produce the mean intra-void number density about 1/5 of the mean external number density of galaxies. The void's population has a lower luminosity and a later morphological type with the medians: M_B = -15.7^m and T = 8 (Sdm), respectively.

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Olga Nasonova, Igor Karachentsev. 2010-11-27. On the kinematics of the Local cosmic void. https://doi.org/10.1007/s10511-011-9153-1

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