The Origins of the Bulk flow

We analyze the origin of the large-scale bulk flow using the CosmicFlows-4 (CF4) peculiar-velocity catalog. We decompose the observed motions into internal components, generated by mass fluctuations within <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mn>200</mml:mn> <mml:msup> <mml:mi>h</mml:mi> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> Mpc, and external ones arising from structures beyond this volume. A weighted-average technique is developed to test the model’s self-consistency while minimizing the impact of non-Gaussian distance errors. The CF4 velocities show excellent agreement with the predicted internal field, yielding <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>β</mml:mi> <mml:mo>=</mml:mo> <mml:mn>0.31</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.01</mml:mn> </mml:mrow> </mml:math> . We also determine that the value of the Hubble constant that should be used for calculating peculiar velocities from the CF4 to be <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:msub> <mml:mi>H</mml:mi> <mml:mn>0</mml:mn> </mml:msub> <mml:mo>=</mml:mo> <mml:mn>75.9</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.1</mml:mn> </mml:mrow> </mml:math> km s Mpc, consistent with CF4 calibrations. Using the minimum-variance formalism, we further separate the bulk flow into its internal and external contributions and find that the observed large-scale bulk flow is dominated by sources beyond <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mn>200</mml:mn> <mml:msup> <mml:mi>h</mml:mi> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> Mpc. The amplitude of this externally driven flow increases monotonically with scale, consistent with the influence of a distant, massive overdensity. We model this overdensity and determine its most likely mass and distance. Our results challenge the commonly made assumption that the flow in our local volume due to external mass concentrations can be modeled as being spatially uniform.

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Journal
The Open Journal of Astrophysics
Published
2026-07-28
DOI
https://doi.org/10.33232/001c.165870
Primary Topic
Galaxies: Formation, Evolution, Phenomena
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article
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article

The Origins of the Bulk flow

Hume A. Feldman, Richard Watkins, Trajan Clark
The Open Journal of Astrophysics
Galaxies: Formation, Evolution, Phenomena
article

The Origins of the Bulk flow

Hume A. Feldman, Richard Watkins, Trajan Clark
article en

Abstract

We analyze the origin of the large-scale bulk flow using the CosmicFlows-4 (CF4) peculiar-velocity catalog. We decompose the observed motions into internal components, generated by mass fluctuations within <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mn>200</mml:mn> <mml:msup> <mml:mi>h</mml:mi> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> Mpc, and external ones arising from structures beyond this volume. A weighted-average technique is developed to test the model’s self-consistency while minimizing the impact of non-Gaussian distance errors. The CF4 velocities show excellent agreement with the predicted internal field, yielding <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>β</mml:mi> <mml:mo>=</mml:mo> <mml:mn>0.31</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.01</mml:mn> </mml:mrow> </mml:math> . We also determine that the value of the Hubble constant that should be used for calculating peculiar velocities from the CF4 to be <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:msub> <mml:mi>H</mml:mi> <mml:mn>0</mml:mn> </mml:msub> <mml:mo>=</mml:mo> <mml:mn>75.9</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.1</mml:mn> </mml:mrow> </mml:math> km s Mpc, consistent with CF4 calibrations. Using the minimum-variance formalism, we further separate the bulk flow into its internal and external contributions and find that the observed large-scale bulk flow is dominated by sources beyond <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mn>200</mml:mn> <mml:msup> <mml:mi>h</mml:mi> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> </mml:mrow> </mml:math> Mpc. The amplitude of this externally driven flow increases monotonically with scale, consistent with the influence of a distant, massive overdensity. We model this overdensity and determine its most likely mass and distance. Our results challenge the commonly made assumption that the flow in our local volume due to external mass concentrations can be modeled as being spatially uniform.

The Open Journal of AstrophysicsVol. 9
Willamette University (US), University of Kansas (US)
Openalex Percentile: Top 98%
Galaxies: Formation, Evolution, Phenomena
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