Pre-explosion, explosion, and post-explosion jets in supernova SN 2019zrk
arXiv:2207.02753 · doi:10.1093/mnras/stac2592
Abstract
I analyse some properties of the luminous transient event SN 2019zrk and conclude that jets were the main powering sources of the pre-explosion outburst (precursor) and ejection of a massive circumstellar matter (CSM), of the very energetic explosion itself, and of the post-explosion bump in the light curve. The pre-explosion energy source is mainly a companion (main sequence, Wolf-Rayet, neutron star or black hole) star that accreted mass and launched jets. I find that the fast expansion of the CSM after acceleration by the explosion ejecta requires the explosion energy to be >10^{52} erg. Only jet-driven explosions can supply this energy in such SN 2009ip-like transients. I conclude that ejecta-CSM interaction is extremely unlikely to power the bright bump at about 110 days after explosion. Instead, I show by applying a jet-driven bump toy-model that post-explosion jets are the most likely explanation for the bump. I leave open the question of whether the explosion itself (main outburst) was a core collapse supernova (CCSN) or a common envelope jets supernova (CEJSN). In this study I further connect peculiar transient events, here 2009ip-like transient events, to CCSNe by arguing that jets drive all events, from regular CCSNe through superluminous CCSNe and to many other peculiar and super-energetic transient events, including CEJSNe. Jet-powering cannot be ignored when analyzing all these types of transients.
arXiv commentAccepted for publication in MNRAS
References in corpus (73)
- Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions
- An enigmatic long-lasting gamma-ray burst not accompanied by a bright supernova
- A two-parameter criterion for classifying the explodability of massive stars by the neutrino-driven mechanism
- Wave-Driven Mass Loss in the Last Year of Stellar Evolution: Setting the Stage for the Most Luminous Core-Collapse Supernovae
- The Unprecedented 2012 Outburst of SN 2009ip: A Luminous Blue Variable Becomes a True Supernova
- Interacting Supernovae and Supernova Impostors. SN 2009ip, is this the end?
- A panchromatic view of the restless SN2009ip reveals the explosive ejection of a massive star envelope
- Discovery of Precursor LBV Outbursts in Two Recent Optical Transients: The Fitfully Variable Missing Links UGC 2773-OT and SN 2009ip
- Common Envelope Evolution Leading to Supernovae with Dense Interaction
- An outburst from a massive star 40 days before a supernova explosion
- Helium Star/Black Hole Mergers: a New Gamma-Ray Burst Model
- The Diversity of Massive Star Outbursts I: Observations of SN 2009ip, UGC 2773 OT2009-1, and Their Progenitors
- SN 2009ip and SN 2010mc: Core-collapse Type IIn supernovae arising from blue supergiants
- Signatures of a jet cocoon in early spectra of a supernova associated with a -ray burst
- Fallback Supernovae: A Possible Origin of Peculiar Supernovae with Extremely Low Explosion Energies
- SN 2009ip á la PESSTO: No evidence for core-collapse yet
- An unusual stellar death on Christmas Day
- Bright, months-long stellar outbursts announce the explosion of interaction-powered supernovae
- Black Hole Accretion Discs and Luminous Transients in Failed Supernovae from Non-Rotating Supergiants
- Hypercritical Accretion, Induced Gravitational Collapse, and Binary-Driven Hypernovae
- A Diversity of Wave-driven Pre-supernova Outbursts
- Explosions Driven by the Coalescence of a Compact Object with the Core of a Massive-Star Companion Inside a Common Envelope: Circumstellar Properties, Light Curves, and Population Statistics
- Exploding Core-Collapse Supernovae with Jittering Jets
- Dead or Alive? Long-term evolution of SN 2015bh (SNhunt275)
- Diversity of common envelope jets supernovae and the fast transient AT2018cow
- Supernovae 2016bdu and 2005gl, and their link with SN 2009ip-like transients: another piece of the puzzle
- Explaining the supernova impostor sn 2009ip as mergerburst
- Clues To The Nature of SN 2009ip from Photometric and Spectroscopic Evolution to Late Times
- Explaining iPTF14hls as a common envelope jets supernova
- Connecting the progenitors, pre-explosion variability, and giant outbursts of luminous blue variables with Gaia16cfr
- Triggering jet-driven explosions of core-collapse supernovae by accretion from convective regions
- SN 2015bh: NGC 2770's 4th supernova or a luminous blue variable on its way to a Wolf-Rayet star?
- Magnetar-powered superluminous supernovae must first be exploded by jets
- Interacting supernovae and supernova impostors. LSQ13zm: an outburst heralds the death of a massive star
- The common envelope jets supernova (CEJSN) r-process scenario
- Wave-driven stellar expansion and binary interaction in pre-supernova outbursts
- Self-regulating jets during the Common Envelope phase
- Angular Momentum Role in the Hypercritical Accretion of Binary-Driven Hypernovae
- Shocked jets in CCSNe can power the zoo of fast blue optical transients
- Disk formation and jet inclination effects in Common Envelopes
- Common envelope jets supernova (CEJSN) impostors resulting from a neutron star companion
- A call for a paradigm shift from neutrino-driven to jet-driven core-collapse supernova mechanisms
- Powering the Second 2012 Outburst of SN 2009ip by Repeating Binary Interaction
- SPH simulations of the induced gravitational collapse scenario of long gamma-ray bursts associated with supernovae
- Applying the Jet Feedback Mechanism to Core-Collapse Supernova Explosions
- A transient radio source consistent with a merger-triggered core collapse supernova
- Jets launched at magnetar birth cannot be ignored
- Common envelope jets supernovae with a black hole companion as possible high energy neutrino sources
- A common envelope jets supernova (CEJSN) impostor scenario for fast blue optical transients
- Observability of inflated companion stars after supernovae in massive binaries
- Explaining Two Recent Intermediate Luminosity Optical Transients (ILOTs) by a Binary Interaction and Jets
- Three-dimensional hydrodynamic simulations of supernova ejecta with a central energy source
- Molecular remnant of Nova 1670 (CK Vulpeculae). II. A three-dimensional view on the gas distribution and velocity field
- Supplying angular momentum to the jittering jets explosion mechanism using inner convection layers
- Photometric and spectroscopic evolution of the interacting transient AT 2016jbu (Gaia16cfr)
- Simulating highly-eccentric common envelope jets supernova (CEJSN) impostors
- Three-dimensional simulations of the jet feedback mechanism in common envelope jets supernova
- Progenitor, environment, and modelling of the interacting transient, AT 2016jbu (Gaia16cfr)
- Emission peaks in the light curve of core collapse supernovae by late jets
- Remnant masses of core collapse supernovae in the jittering jets explosion mechanism
- Simulating the negative jet feedback mechanism in common envelope jets supernovae
- Powering luminous core collapse supernovae with jets
- Accelerating very fast gas in the supernova impostor sn 2009ip with jets from a stellar companion
- The magnetar model of the superluminous supernova GAIA16apd and the explosion jet feedback mechanism (JFM)
- Double common envelope jets supernovae (CEJSNe) by triple-star systems
- Signatures of an eruptive phase before the explosion of the peculiar core-collapse SN 2013gc
- Pre-supernova outbursts of massive stars in the presence of a neutron star companion
- Neutrino Emission from Luminous Fast Blue Optical Transients
- Fast Ejecta Resulted from Jet-Wind Interaction in the Great Eruption of Eta Carinae
- Simulating jets from a neutron star companion hours after a core collapse supernova
- AT2018lqh: Black Hole Born from a Rotating Star?
- Post-explosion positive jet-feedback activity in inner ejecta of core collapse supernovae
- Simulating the outcome of binary neutron star merger in common envelope jets supernovae