A gravitational acceleration model to explain the double-peaked narrow emission lines shifted in the same direction
XingQian Chen, GuiLin Liao, Qi Zheng, and XueGuang Zhang

TL;DR
This paper introduces a gravitational acceleration model to explain why some double-peaked narrow emission lines are shifted in the same direction, suggesting a new interpretation for these spectral features in merging galaxy systems.
Contribution
The paper presents the first gravitational acceleration model for same-direction shifted double-peaked emission lines in merging dual-core galaxies, supported by simulations and a real galaxy case.
Findings
Probability of same-direction shifts is 5.81% in merging systems.
Simulation results support the gravitational acceleration explanation.
Identified a galaxy consistent with the model's predictions.
Abstract
In this manuscript, we propose, for the first time, an oversimplified but potentially effective gravitational acceleration model to interpret the double-peaked narrow emission lines (DPNELs) shifted in the same direction. We adopt the framework of a merging kpc-scale dual-core system in an elliptical orbit, which has an emission-line galaxy with clear narrow line regions (NLRs) merging with a companion galaxy lacking emission line features. Due to gravitational forces induced by both galaxies on the NLRs, the accelerations of the far-side and near-side NLR components may share the same vector direction when projected along the line-of-sight, leading the velocities of the observed DPNELs to shift in the same direction. Our simulations indicate that the probability of producing double-peaked features shifted in the same direction reaches 5.81% in merging kpc-scale dual core systems…
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Taxonomy
TopicsScientific Research and Discoveries · Dark Matter and Cosmic Phenomena · Particle Detector Development and Performance
