The roles of jets: CF, CCSN, PN, CEE, GEE, ILOT
Noam Soker (Technion, Haifa)

TL;DR
This paper reviews the role of jet-inflated bubbles across various astrophysical systems, emphasizing the negative jet feedback mechanism and its failures leading to energetic phenomena like gamma-ray bursts and supernovae.
Contribution
It provides a comprehensive overview of jet-inflated bubbles in different astrophysical contexts and discusses the impact of feedback mechanism failures on energetic cosmic events.
Findings
Jets inflate bubbles in multiple systems like clusters and nebulae.
Failure of jet feedback can lead to energetic phenomena such as gamma-ray bursts.
Jets influence the evolution and outcomes of various astrophysical objects.
Abstract
I review the roles of jet-inflated bubbles in determining the evolution of different astrophysical objects. I discuss astrophysical systems where jets are known to inflate bubbles (cooling flow [CF] clusters; young galaxies; intermediate luminosity optical transients [ILOTs]; bipolar planetary nebulae [PNe]), and systems that are speculated to have jet-inflated bubbles (core collapse supernovae [CCSNe]; common envelope evolution [CEE]; grazing envelope evolution [GEE]). The jets in many of these cases act through a negative jet feedback mechanism (JFM). I discuss the outcomes when the JFM fizzle, or does not work at all. According to this perspective, some very interesting and energetic events owe their existence to the failure of the JFM, including stellar black holes, gamma ray bursts, and type Ia supernovae.
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