Long-term evolution of a supernova remnant hosting a double neutron star binary

Abstract

An ultra-stripped supernova (USSN) is a type of core-collapse SN explosion proposed to be a candidate formation site of a double neutron star (DNS) binary. We investigate the dynamical evolution of an ultra-stripped supernova remnant (USSNR), which should host a DNS at its center. By accounting for the mass-loss history of the progenitor binary using a model developed by a previous study, we construct the large-scale structure of the {circumstellar medium (CSM)} up to a radius $\sim 100\mathrm{pc}$, and simulate the explosion and subsequent evolution of a USSN surrounded by such a CSM environment. We find that the CSM encompasses an extended region characterized by a hot plasma with a temperature $\sim 10^8$K located around the termination shock of the wind from the progenitor binary ($\sim 10$pc), and the USSNR blastwave is drastically weakened while penetrating through this hot plasma. Radio continuum emission from a young USSNR is sufficiently bright to be detectable if it inhabits our Galaxy but faint compared to the observed Galactic SNRs, and thereafter declines in luminosity through adiabatic cooling. Within our parameter space, USSNRs typically exhibit a low radio luminosity and surface brightness compared to the known Galactic SNRs. Due to the small event rate of USSNe and their relatively short observable lifespan, we calculate that USSNRs account for only $\sim 0.1$-$1$ % of the total SNR population. This is consistent with the fact that no SNR hosting a DNS binary has been discovered in the Milky Way so far.

arXiv comment23 pages, 10 figures, 3 tables, accepted for publication in The Astrophysical Journal

References in corpus (71)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• The Zwicky Transient Facility: System Overview, Performance, and First Results
• Common Envelope Evolution: Where we stand and how we can move forward
• An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system
• The Zwicky Transient Facility: Science Objectives
• Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
• A "kilonova" associated with short-duration gamma-ray burst 130603B
• Formation of Double Neutron Star Systems
• Simulations of Ion Acceleration at Non-relativistic Shocks. I. Acceleration Efficiency
• Radiative Transfer Simulations for Neutron Star Merger Ejecta
• Type Ib/c supernovae in binary systems I. Evolution and properties of the progenitor stars
• Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817
• Circumstellar Emission from Type Ib and Ic Supernovae
• The death of massive stars - II. Observational constraints on the progenitors of type Ibc supernovae
• A revised catalogue of 294 Galactic supernova remnants
• Simultaneous Acceleration of Protons and Electrons at Nonrelativistic Quasiparallel Collisionless Shocks
• Ultra-stripped Type Ic supernovae from close binary evolution
• Radio Emission and Particle Acceleration in SN 1993J
• Radio emission from Supernova Remnants
• The Evolution of Supernovae in Circumstellar Wind-Blown Bubbles I. Introduction and One-Dimensional Calculations
• Simulations and Theory of Ion Injection at Non-relativistic Collisionless Shocks
• Radio and X-Ray Emission as Probes of Type IIP Supernovae and Red Supergiant Mass Loss
• The X-ray synchrotron emission of RCW 86 and the implications for its age
• Shock acceleration efficiency in radio relics
• The Double Pulsar J0737--3039: Testing the Neutron Star Equation of State
• The Evolution of Supernovae in Circumstellar Wind Bubbles II: Case of a Wolf-Rayet star
• Progenitor models of the electromagnetic transient associated with the short GRB 130603B
• The Fast and Furious Decay of the Peculiar Type Ic Supernova 2005ek
• A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
• On the Expansion Rate, Age, and Distance of the Supernova Remnant G266.2-1.2 (Vela Jr.)
• Neutrino-driven explosions of ultra-stripped type Ic supernovae generating binary neutron stars
• Radio and X-ray observations of SN 2006jd: Another strongly interacting Type IIn supernova
• The radio surface brightness to diameter relation for galactic supernova remnants: sample selection and robust analysis with various fitting offsets
• Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars
• Multi-D Simulations of Ultra-Stripped Supernovae to Shock Breakout
• Asymmetries in the Type IIn SN2010jl
• A Multi-Frequency Radio Study of Supernova Remnant G292.0+1.8 and its Pulsar Wind Nebula
• The First Measurement of Cassiopeia A's Forward Shock Expansion Rate
• A Late-Time Flattening of Light Curves in Gamma-Ray Burst Afterglows
• Broad-band Observations and Modeling of the Shell-Type Supernova Remnant G347.3-0.5
• Radii and Mass-loss Rates of Type IIb Supernova Progenitors
• Density probability distribution functions of diffuse gas in the Milky Way
• Recombining Plasma and Hard X-ray Filament in the Mixed-Morphology Supernova Remnant W44
• A Generalized Model of Nonlinear Diffusive Shock Acceleration Coupled to an Evolving Supernova Remnant
• SN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova
• Proton Acceleration in Weak Quasi-parallel Intracluster Shocks: Injection and Early Acceleration
• Supernova remnant W49B and its environment
• A Chandra Observation of Supernova Remnant G350.1-0.3 and Its Central Compact Object
• A high resolution HI study towards the supernova remnant Puppis A and its environments
• Injection and Acceleration of Electrons at A Strong Shock: Radio and X-ray Study of Young Supernova 2011dh
• Supernova ejecta interacting with a circumstellar disk. I. two-dimensional radiation-hydrodynamic simulations
• Eleven years of radio monitoring of the Type IIn supernova SN 1995N
• Radio emission of SN1993J. The complete picture: II. Simultaneous fit of expansion and radio light curves
• G309.2-00.6 and jets in supernova remnants
• Properties of the post in-spiral common envelope ejecta I: dynamical and thermal evolution
• Explosive nucleosynthesis of ultra-stripped Type Ic supernovae: application to light trans-iron elements
• Two Distinct-Absorption X-Ray Components from Type IIn Supernovae: Evidence for Asphericity in the Circumstellar Medium
• On the observational behaviour of the highly polarized Type IIn supernova SN 2017hcc
• Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs
• Two New Ejecta-Dominated Galactic Supernova Remnants: G337.2-0.7 and G309.2-0.6
• 3D simulations of the non-thermal broad-band emission from young supernova remnants including efficient particle acceleration
• Radio Emission from Supernovae in the Very Early Phase: Implications for the Dynamical Mass Loss of Massive Stars
• Time evolution of broadband non-thermal emission from supernova remnants in different circumstellar environments
• Modeling of interactions between supernovae ejecta and aspherical circumstellar environments
• Exploring the X-ray emission properties of the supernova remnant G67.7+1.8 and its central X-ray sources
• Infrared and X-ray study of the Galactic SNR G15.9+0.2
• Exploring the supernova remnant G308.4-1.4
• The rate of iPTF 14gqr like ultra-stripped supernovae and binary evolution leading to double neutron star formation
• Radio Emission from Ultra-stripped Supernovae as Diagnostics for Properties of the Remnant Double Neutron Star Binaries
• Ejecta detection in the middle-aged Galactic supernova remnant G296.1-0.5 observed with Suzaku