Resolved simulations of jet–ISM interaction: Implications for gas dynamics and star formation-Reference-Cited by-同舟云学术

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Resolved simulations of jet–ISM interaction: Implications for gas dynamics and star formation

Published:2021-11 Issue:9-10 Volume:342 Page:1140-1145
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron Nachr

Author:

Mukherjee Dipanjan¹^ORCID,Bicknell Geoffrey V.²,Wagner Alexander Y.³^ORCID

Affiliation:

1. Inter‐University Centre for Astronomy and Astrophysics (IUCAA) Pune University Pune India

2. Research School of Astronomy and Astrophysics Australian National University Canberra Australian Capital Territory Australia

3. Center for Computational Sciences University of Tsukuba Tsukuba Japan

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210061

Reference58 articles.

1. DISCOVERY OF AN ACTIVE GALACTIC NUCLEUS DRIVEN MOLECULAR OUTFLOW IN THE LOCAL EARLY-TYPE GALAXY NGC 1266

2. SUPPRESSION OF STAR FORMATION IN NGC 1266

3. Unification of the Radio and Optical Properties of Gigahertz Peak Spectrum and Compact Steep‐Spectrum Radio Sources

4. Jet‐induced Emission‐Line Nebulosity and Star Formation in the High‐Redshift Radio Galaxy 4C 41.17

5. GPS and CSS Sources — Theory and Modelling

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1. Molecular Gas Kinematics in Local Early-Type Galaxies with ALMA;Galaxies;2024-07-02

2. JWST discovers an AGN ionization cone but only weak radiatively driven feedback in a powerful z ≈ 3.5 radio-loud AGN;Astronomy & Astrophysics;2024-03

3. Probing the two-body decaying dark matter scenario with weak lensing and the cosmic microwave background;Astronomy & Astrophysics;2024-03

4. Numerical modelling of the lobes of radio galaxies – Paper V: universal pressure profile cluster atmospheres;Monthly Notices of the Royal Astronomical Society;2023-09-26

5. Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters;Galaxies;2023-06-13

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