The DOI matches its Crossref record; 92 of the 92 references it cites were found in a registry or an index.
Relativistic jet feedback – III. Feedback on gas discs
Open accessAbstract
We study the interactions of a relativistic jet with a dense turbulent gaseous disc of radius ∼2 kpc. We have performed a suite of simulations with different mean density, jet power, and orientation. Our results show that: (A) The relativistic jet couples strongly with the gas in the inner kpc, creating a cavity and launching outflows. (B) The high pressure bubble inflated by the jet and its back-flow compresses the disc at the outer edges, driving inflows within the disc. (C) Jets inclined towards the disc affect the disc more and launch sub-relativistic, wide-angled outflows along the minor axis. (D) Shocks driven directly by the jet and the jet-driven energy bubble raise the velocity dispersion throughout the disc by several times its initial value. (E) Compression by the jet-driven shocks can enhance the star formation rate in the disc, especially in a ring-like geometry close to the axis. However, enhanced turbulent dispersion in the disc also leads to quenching of star formation. Whether positive or negative feedback dominates depends on jet power, ISM density, jet orientation with respect to the disc, and the time-scale under consideration. Qualitatively, our simulations compare favourably with kinematic and morphological signatures of several observed galaxies such as NGC 1052, NGC 3079, 3C 326, and 3C 293.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
The Global Schmidt Law in Star‐forming Galaxies
Kennicutt, Jr. (1998) · The Astrophysical Journal · doi:10.1086/305588 · Cited by 5,202
The Piecewise Parabolic Method (PPM) for gas-dynamical simulations
Colella, P., & Woodward, P. R. (1984) · Journal of Computational Physics · doi:10.1016/0021-9991(84)90143-8 · Cited by 3,954
Croton, D. J., Springel, V., White, S. D. M., De Lucia, G., Frenk, C. S., Gao, L., Jenkins, A., Kauffmann, G., Navarro, J. F., & Yoshida, N. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09675.x · Cited by 3,685
Energy input from quasars regulates the growth and activity of black holes and their host galaxies
Di Matteo, T., Springel, V., & Hernquist, L. (2005) · Nature · doi:10.1038/nature03335 · Cited by 3,353
On the Gravitational Stability of a Disk of Stars
Toomre, A. (1964) · The Astrophysical Journal · doi:10.1086/147861 · Cited by 3,349 · cited 1×
“A gas disk is will be gravitationally stable if Q > 1 (Toomre 1964; Wang & Silk 1994).”
BackgroundObservational Evidence of Active Galactic Nuclei Feedback
Fabian, A. C. (2012) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081811-125521 · Cited by 2,795
Breaking the hierarchy of galaxy formation
Bower, R. G., Benson, A. J., Malbon, R., Helly, J. C., Frenk, C. S., Baugh, C. M., Cole, S., & Lacey, C. G. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.10519.x · Cited by 2,464
Springel, V., & Hernquist, L. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06206.x · Cited by 2,262
Interstellar bubbles. II - Structure and evolution
Weaver, R., McCray, R., Castor, J., Shapiro, P., & Moore, R. (1977) · The Astrophysical Journal · doi:10.1086/155692 · Cited by 1,736 · cited 1×
“…(5− β)3(3− β) 6π(7− 2β)(11− β) ](2−β)/(5−β) ×R−3β/(5−β)c ρ3/(5−β)c F (2−β)/(5−β) E t −(β+4)/(5−β) (A11) pB = 3(7− 2β) (3− β)(5− β)2 [ (3− β)(5− β)3 6π(7− 2β)(11− β) ]2/3 × ρ1/3c Rβ/3c F 2/3R −(β+4)/3 B (A12) For β = 0 the above equations reduce to the expressions derived in Weaver et al.…”
PLUTO: A Numerical Code for Computational Astrophysics
Mignone, A., Bodo, G., Massaglia, S., Matsakos, T., Tesileanu, O., Zanni, C., & Ferrari, A. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/513316 · Cited by 1,634
Cited by
Cool outflows in galaxies and their implications
Veilleux, S., Maiolino, R., Bolatto, A. D., & Aalto, S. (2020) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-019-0121-9 · Cited by 466
The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way
Sarkar, K. C. (2024) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-024-00152-1 · Cited by 34
“Possible mechanisms of jet dissipation are i) magnetic kink instability (Tchekhovskoy & Bromberg 2016), or ii) interaction with dense clouds (Mukherjee et al. 2018; Cecil et al. 2021).”
BackgroundWhat drives the growth of black holes: A decade of progress
Alexander, D. M., Hickox, R. C., Aird, J., Combes, F., Costa, T., Habouzit, M., Harrison, C. M., Leng, R. I., Morabito, L. K., Uckelman, S. L., et al. (2025) · New Astronomy Reviews · doi:10.1016/j.newar.2025.101733 · Cited by 18
Dissipation of AGN jets in a clumpy interstellar medium
Dutta, R., Sharma, P., Sarkar, K. C., & Stone, J. M. (2024) · arXiv · doi:10.48550/arxiv.2401.00446 · Cited by 18
Misaligned Jets from Sgr A* and the Origin of Fermi/eROSITA Bubbles
Sarkar, K. C., Mondal, S., Sharma, P., & Piran, T. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/acd75d · Cited by 17
Metadata
- Authors
- Mukherjee, D., Bicknell, G. V., Wagner, A. Y., Sutherland, R. S., & Silk, J.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2018-07-05
- Volume
- 479
- Issue
- 4
- Pages
- 5544-5566
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2792905005
- Cited by
- 257
- References
- 92
- FWCI
- 10.66
- Type
- journal article
- Language
- en
- Open access
- green
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Relativistic jet feedback – III. Feedback on gas discs. https://app.cochat.ai/papers/10.1093/mnras/sty1776
- The paper
- Mukherjee, D., Bicknell, G. V., Wagner, A. Y., Sutherland, R. S., & Silk, J. (2018). Relativistic jet feedback – III. Feedback on gas discs. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/sty1776
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.