pith. sign in

arxiv: astro-ph/0312282 · v1 · submitted 2003-12-10 · 🌌 astro-ph

Jet-Induced Star Formation

classification 🌌 astro-ph
keywords formationgalaxiesjet-inducedradiostardensefr-igalaxy
0
0 comments X
read the original abstract

Jets from radio galaxies can have dramatic effects on the medium through which they propagate. We review observational evidence for jet-induced star formation in low ('FR-I') and high ('FR-II') luminosity radio galaxies, at low and high redshifts respectively. We then discuss numerical simulations which are aimed to explain a jet-induced starburst ('Minkowski's Object') in the nearby FR-I type radio galaxy NGC 541. We conclude that jets can induce star formation in moderately dense (10 cm-3), warm (10,000 K) gas; that this may be more common in the dense environments of forming, active galaxies; and that this may provide a mechanism for 'positive' feedback from AGN in the galaxy formation process.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. PEARLS: Two Distinct Populations of AGN Hosts Moving Between Star Formation and Quiescence

    astro-ph.GA 2026-05 unverdicted novelty 4.0

    NIRCam-selected AGN hosts split into a 'bridge' group with moderate-to-low SFRs and a 'branch' group above the SFMS with SFR rising with AGN fraction; both populations show recent transitions between star formation an...