English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

I review the roles of jet-inflated bubbles in determining the evolution ofdifferent astrophysical objects. I discuss astrophysical systems where jets areknown 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 (corecollapse supernovae [CCSNe]; common envelope evolution [CEE]; grazing envelopeevolution [GEE]). The jets in many of these cases act through a negative jetfeedback mechanism (JFM). I discuss the outcomes when the JFM fizzle, or doesnot work at all. According to this perspective, some very interesting andenergetic events owe their existence to the failure of the JFM, includingstellar black holes, gamma ray bursts, and type Ia supernovae.

The roles of jets: CF, CCSN, PN, CEE, GEE, ILOT