Inhomogeneities and the modeling of radio supernovae
arXiv:1704.05283 · doi:10.3847/1538-4357/aa6cad
Abstract
Observations of radio supernovae often exhibit characteristics not readily accounted for by a homogeneous, spherically symmetric synchrotron model; e.g., flat-topped spectra/lightcurves. It is shown that many of these deviations from the standard model can be attributed to an inhomogeneous source structure. It is argued that the radio emission in Type Ib/c supernovae has a small volume filling factor and comes from a narrow region associated with the forward shock, while the radio emission region in SN 1993J (Type IIb) is determined by the extent of the Rayleigh-Taylor instability emanating from the contact discontinuity. Attention is also drawn to the similarities between radio supernovae and the structural properties of supernova remnants.
21 pages, 4 figures. Accepted to ApJ
References in corpus (8)
- Simultaneous Acceleration of Protons and Electrons at Nonrelativistic Quasiparallel Collisionless Shocks
- Simulations and Theory of Ion Injection at Non-relativistic Collisionless Shocks
- Simulations of Ion Acceleration at Non-relativistic Shocks. III. Particle Diffusion
- Long Term Radio Monitoring of SN 1993J
- Magnetic-Field Amplification in the Thin X-ray Rims of SN1006
- Energy Dependence of Synchrotron X-Ray Rims in Tycho's Supernova Remnant
- Imaging the Expanding Shell of SN 2011dh
- Joining radio with X-rays: A revised model for SN 1993J
Cited by in corpus (19)
- Fast Radio Bursts: An Extragalactic Enigma
- Delayed Radio Flares from a Tidal Disruption Event
- The Radio Luminosity-Risetime Function of Core-Collapse Supernovae
- Cosmic ray production in supernovae
- Core collapse supernovae as Cosmic Ray sources
- Performance of a highly sensitive, 19-element, dual-polarization, cryogenic L-band Phased Array Feed on the Green Bank Telescope
- Thermal Electrons in Mildly-relativistic Synchrotron Blast-waves
- uGMRT observations of a Fast and Blue Optical Transient -- AT 2018cow
- The Deepest Radio Observations of Nearby Type IA Supernovae: Constraining Progenitor Types and Optimizing Future Surveys
- Late-Time Evolution and Modeling of the Off-Axis Gamma-ray Burst Candidate FIRST J141918.9+394036
- Type Ib supernova Master OT J120451.50+265946.6: radio emitting shock with inhomogeneities crossing through a dense shell
- The nascent milliquasar VT J154843.06+220812.6: tidal disruption event or extreme accretion-state change?
- Stochastic re-acceleration and magnetic-field damping in Tycho's supernova remnant
- The dense and non-homogeneous circumstellar medium revealed in radio wavelengths around the Type Ib SN 2019oys
- Radio evolution of a Type IIb supernova SN 2016gkg
- Circular polarisation in compact radio sources: Constraints on particle acceleration and electron-positron pairs
- The radio spectra of SN 2020oi: Effects of radiative cooling on the deduced source properties
- The X-ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-Driven Massive Star Explosions
- Implications of the low frequency turn-over in the spectrum of radio knot C in DG Tau