SIMBAD references

2007ApJ...655L..41U - Astrophys. J., 655, L41-L44 (2007/January-3)

An analysis of the broadband (22-3900 MHz) radio spectrum of HB 3 (G132.7+1.3): the detection of thermal radio emission from an evolved supernova remnant?

UROSEVIC D., PANNUTI T.G. and LEAHY D.

Abstract (from CDS):

We present an analysis of the broadband radio spectrum (from 22 to 3900 MHz) of the Galactic supernova remnant (SNR) HB 3 (G132.7+1.3). Published observations have revealed that a curvature is present in the radio spectrum of this SNR, indicating that a single synchrotron component appears insufficient to adequately fit the spectrum. We present here a fit to this spectrum using a combination of a synchrotron component and a thermal bremsstrahlung component. We discuss properties of the latter component and estimate the ambient density implied by the presence of this component to be n∼10/cm3. We have also analyzed X-ray spectra extracted from archived ASCA GIS observations of different regions of HB 3 to obtain independent estimates of the density of the surrounding interstellar medium (ISM). From this analysis, we have derived electron densities of (0.1-0.4)f–1/2/cm3 for the ISM for the three different regions of the SNR, where f is the volume filling factor. By comparing these density estimates with the estimate derived from the thermal bremsstrahlung component, we argue that the radio thermal bremsstrahlung emission is emitted from a thin shell enclosing HB 3. The presence of this thermal bremsstrahlung component in the radio spectrum of HB 3 suggests that this SNR is in fact interacting with an adjacent molecular cloud associated with the H II region W3. By extension, we argue that the presence of thermal emission at radio wavelengths may be a useful tool for identifying interactions between SNRs and molecular clouds, and for estimating the ambient density near SNRs using radio continuum data.

Abstract Copyright:

Journal keyword(s): ISM: individual (G132.7+1.3) - ISM: individual (HB 3) - Radiation Mechanisms: Thermal - Radio Continuum: General - ISM: Supernova Remnants

Simbad objects: 2

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2019.10.14-14:32:58

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