Probing Interstellar Dust with Infrared Echoes from the Cas A Supernova

TL;DR

This study models the infrared echo spectrum near Cas A to understand interstellar dust processing, revealing PAH destruction and dehydrogenation caused by supernova UV bursts, and demonstrates the potential of infrared echoes for ISM research.

Contribution

The paper develops a detailed dust emission model based on SN 1993J data to interpret the infrared echo spectrum of Cas A, highlighting dust processing effects.

Findings

PAHs with fewer than 300 carbon atoms are absent, indicating destruction by UV burst.

Infrared spectrum is consistent with strongly dehydrogenated PAHs.

Estimated echo region density is around 680 H cm^{-3}.

Abstract

We present the analysis of an IRS 5-38 {\mu}m spectrum and MIPS photometric measurements of an infrared echo near the Cassiopeia A supernova remnant observed with the Spitzer Space Telescope. We have modeled the recorded echo accounting for PAHs, quantum-heated carbon and silicate grains, as well as thermal carbon and silicate particles. Using the fact that optical light echo spectroscopy has established that Cas A originated from a type IIb supernova explosion showing an optical spectrum remarkably similar to the prototypical type IIb SN 1993J, we use the latter to construct template data input for our simulations. We are then able to reproduce the recorded infrared echo spectrum by combining the emission of dust heated by the UV burst produced at the shock breakout after the core-collapse and dust heated by optical light emitted near the visual maximum of the supernova light curve, where the UV burst and optical light curve characteristics are based on SN 1993J. We find a mean density of \sim680 H cm^{-3} for the echo region, with a size of a few light years across. We also find evidence of dust processing in the form of a lack of small PAHs with less than \sim300 carbon atoms, consistent with a scenario of PAHs destruction by the UV burst via photodissociation at the estimated distance of the echo region from Cas A. Furthermore, our simulations suggest that the weak 11 {\mu}m features of our recorded infrared echo spectrum are consistent with a strong dehydrogenated state of the PAHs. This exploratory study highlights the potential of investigating dust processing in the interstellar medium through infrared echoes.