Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution

I argue that the high percentage of planetary nebulae (PNe) that are shaped by jets show that main sequence stars in binary systems can accrete mass at a high rate from an accretion disk and launch jets. Not only does this allow jets to shape PNe, but this also points to the importance of jets in ot...

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Main Author: Noam Soker
Format: Article
Language:English
Published: MDPI AG 2020-03-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/8/1/26
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author Noam Soker
author_facet Noam Soker
author_sort Noam Soker
collection DOAJ
description I argue that the high percentage of planetary nebulae (PNe) that are shaped by jets show that main sequence stars in binary systems can accrete mass at a high rate from an accretion disk and launch jets. Not only does this allow jets to shape PNe, but this also points to the importance of jets in other types of binary systems and in other processes. These processes include the grazing envelope evolution (GEE), the common envelope evolution (CEE), and the efficient conversion of kinetic energy to radiation in outflows. Additionally, the jets point to the possibility that many systems launch jets as they enter the CEE, possibly through a GEE phase. The other binary systems in which jets might play significant roles include intermediate-luminosity optical transients (ILOTs), supernova impostors (including pre-explosion outbursts), post-CEE binary systems, post-GEE binary systems, and progenitors of neutron star binary systems and black hole binary systems. One of the immediate consequences is that the outflow of these systems is highly-non-spherical, including bipolar lobes, jets, and rings.
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spelling doaj.art-31b85ac54d3c41a68661a16e93f5f5c62022-12-21T23:53:58ZengMDPI AGGalaxies2075-44342020-03-01812610.3390/galaxies8010026galaxies8010026Shaping Planetary Nebulae with Jets and the Grazing Envelope EvolutionNoam Soker0Department of Physics, Technion, Haifa 3200003, IsraelI argue that the high percentage of planetary nebulae (PNe) that are shaped by jets show that main sequence stars in binary systems can accrete mass at a high rate from an accretion disk and launch jets. Not only does this allow jets to shape PNe, but this also points to the importance of jets in other types of binary systems and in other processes. These processes include the grazing envelope evolution (GEE), the common envelope evolution (CEE), and the efficient conversion of kinetic energy to radiation in outflows. Additionally, the jets point to the possibility that many systems launch jets as they enter the CEE, possibly through a GEE phase. The other binary systems in which jets might play significant roles include intermediate-luminosity optical transients (ILOTs), supernova impostors (including pre-explosion outbursts), post-CEE binary systems, post-GEE binary systems, and progenitors of neutron star binary systems and black hole binary systems. One of the immediate consequences is that the outflow of these systems is highly-non-spherical, including bipolar lobes, jets, and rings.https://www.mdpi.com/2075-4434/8/1/26planetary nebulae: generalism: jets and outflowsstars: agb and post-agbbinaries: generalstars: mass-lossstars: windsstars: outflows
spellingShingle Noam Soker
Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution
Galaxies
planetary nebulae: general
ism: jets and outflows
stars: agb and post-agb
binaries: general
stars: mass-loss
stars: winds
stars: outflows
title Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution
title_full Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution
title_fullStr Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution
title_full_unstemmed Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution
title_short Shaping Planetary Nebulae with Jets and the Grazing Envelope Evolution
title_sort shaping planetary nebulae with jets and the grazing envelope evolution
topic planetary nebulae: general
ism: jets and outflows
stars: agb and post-agb
binaries: general
stars: mass-loss
stars: winds
stars: outflows
url https://www.mdpi.com/2075-4434/8/1/26
work_keys_str_mv AT noamsoker shapingplanetarynebulaewithjetsandthegrazingenvelopeevolution