Thermal radio absorption as a tracer of the interaction of SNRs with their environments
arXiv:2108.08178 · doi:10.1051/0004-6361/202141635
Abstract
We present new images and continuum spectral analysis for 14 resolved Galactic SNRs selected from the 74 MHz Very Large Array Low-Frequency Sky Survey Redux (VLSSr). We combine new integrated measurements from the VLSSr with flux densities extracted from the GLEAM and measurements from the literature to generate improved continuum spectra. We combine the VLSSr images with publicly available images at 1.4 GHz, to analyse the resolved morphology and spectral index distribution across each SNR. Three of the SNRs, Kepler, G28.6-0.1, and Tycho, have integrated spectra which can be adequately fit with simple power laws. The resolved spectral index map for Tycho confirms internal absorption which was previously detected by the LOFAR, but it is insufficient to affect the fit to the integrated spectrum. For the pulsar wind nebulae G21.5-0.9 and 3C58 we identify high-frequency spectral breaks at 38 and 12 GHz, respectively. A low frequency spectral turnover adequately fits the data of the remaining nine SNRs. For Kes 67, Kes 69, Kes75, and 3C397, we attribute the absorption to ionised gas along the line of sight, possibly from extended HII region envelopes. For W41 the absorption can be attributed to HII regions located in its immediate proximity. Thermal absorption from interactions at the ionised interface between SNR forward shocks and the surrounding medium were previously identified as responsible for the low frequency turnover in SNR 3C391; our integrated spectrum is consistent with the previous results. We present evidence for the same phenomenon in three additional SNRs, Kes73, W49B, and 3C396, and derive constraints on the physical properties of the interaction. This result indicates that interactions between SNRs and their environs should be readily detectable through thermal absorption by future low frequency observations of SNRs with improved sensitivity and resolution.
Accepted for publication in Astronomy and Astrophysics (on August 14th 2021), 29 pages, 8 figures (the quality of the figures has been degraded), 17 tables
References in corpus (33)
- The LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release
- The Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey
- The VLA Low-frequency Sky Survey
- The VLA Galactic Plane Survey
- The Very Large Array Low-frequency Sky Survey Redux (VLSSr)
- Discovery of 35 New Supernova Remnants in the Inner Galaxy
- The Electron Temperature Gradient in the Galactic Disk
- The 74MHz System on the Very Large Array
- The LOFAR LBA Sky Survey I. survey description and preliminary data release
- A Near-Infrared and X-ray Study of W49B: A Wind Cavity Explosion
- Radio Images of 3C 58: Expansion and Motion of its Wisp
- The Distances of SNR W41 and overlapping HII regions
- The Expansion and Radio Spectral Index of G21.5-0.9: Is PSR J1833-1034 the Youngest Pulsar?
- VLA and XMM-Newton observations of the SNR W41/TeV Gamma-ray source HESS J1834-087
- GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey II: Galactic Plane ,
- The Density and Mass of Unshocked Ejecta in Cassiopeia A through Low Frequency Radio Absorption
- NuSTAR study of Hard X-Ray Morphology and Spectroscopy of PWN G21.5-0.9
- Cosmic ray acceleration at perpendicular shocks in supernova remnants
- On the radio spectra of supernova remnants
- Supernova remnant W49B and its environment
- 74 MHz Discrete HII Absorption Regions Towards The Inner Galaxy
- Near-infrared [Fe II] and H Emission-line Study of Galactic Supernova Remnants in the First Quadrant
- Expansion of Kes 73, a Shell Supernova Remnant Containing a Magnetar
- High-resolution Near-infrared Spectroscopic Study of Galactic Supernova Remnants. I. Kinematic Distances
- On the broad-band synchrotron spectra of pulsar wind nebulae
- 3D simulations of the non-thermal broad-band emission from young supernova remnants including efficient particle acceleration
- Massive stars in the giant molecular cloud G23.3-0.3 and W41
- Low-frequency radio absorption in Tycho's supernova remnant
- A 4-6 GHz Radio Recombination Line Survey in the Milky Way
- Stochastic re-acceleration and magnetic-field damping in Tycho's supernova remnant
- The Interaction Between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30
- A more detailed look at Galactic magnetic field models: using free-free absorption in HII regions
- A Study of Fermi-LAT GeV gamma-ray Emission towards the Magnetar-harboring Supernova Remnant Kesteven 73 and Its Molecular Environment
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- GaLactic and Extragalactic All-sky Murchison Widefield Array survey eXtended (GLEAM-X) III: Galactic Plane
- Polarized Emission From Four Supernova Remnants In The THOR Survey
- HAWC Study of Very-High-Energy -ray Spectrum of HAWC J1844-034
- Multi-antenna probing of absorbing regions inside and outside Cassiopeia A
- GaLactic and Extragalactic All-sky Murchison Widefield Array survey eXtended (GLEAM-X) I: Survey Description and Initial Data Release
- Broadband radio study of the supernova remnant Kes 73