Issue |
A&A
Volume 694, February 2025
|
|
---|---|---|
Article Number | A217 | |
Number of page(s) | 5 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/202452567 | |
Published online | 14 February 2025 |
Velocity shift of a C IV broad absorption line in quasar SDSS J145229.08+093204.9
1
School of Information Engineering, Baise University, Baise 533000, China
2
College of Chemical and Environmental Engineering, Baise University, Baise 533000, China
⋆ Corresponding author; yingru_lin@qq.com
Received:
10
October
2024
Accepted:
23
January
2025
We present the observation of a velocity shift in the broad absorption line (BAL) of C IV ion in quasar SDSS J145229.08+093204.9 (hereafter J1452+0932).This quasar exhibits three distinct BAL systems, designated as systems A, B, and C. Notably, system A, which possesses the highest velocity of approximately −23 000 km s−1, demonstrates a velocity shift of −1097 km s−1 in its C IV ion over a rest-frame period of approximately 1.7 years. To elucidate the nature of these variations, we conducted a comprehensive analysis focusing on the variation situation, location, ionisation state, and profile shape of the three BAL systems in J1452+0932. Our findings reveal that system A is situated closer to the central source compared to systems B and C. Furthermore, system A exhibits higher velocities, higher ionisation states, and smoother profile morphologies. These characteristics collectively suggest that the outflow generating system A is situated in a particularly extreme environment and experiences more pronounced impacts from background radiation energy than systems B and C. Consequently, we postulate that the observed velocity shift in system A may signify an actual line-of-sight acceleration of the outflow, induced by the radiation pressure emanating from the central source. Specifically, this scenario could occur if our line of sight intersects an outflow at a location where it is undergoing acceleration towards its terminal outflow velocity, or if a previously coasting outflow is undergoing renewed acceleration.
Key words: galaxies: active / quasars: absorption lines / quasars: individual: SDSS J145229.08+093204.9
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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