Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A

TL;DR

This study investigates the interstellar medium around supernova remnant Puppis A using multi-wavelength data, revealing shock interactions, supporting a hadronic gamma-ray origin, and estimating the remnant's age and cosmic-ray energy.

Contribution

It provides a comprehensive multi-wavelength analysis of Puppis A, linking ISM properties with gamma-ray emission and estimating the remnant's age and cosmic-ray energy.

Findings

ISM is dense, clumpy, mainly in the northeast of the SNR.

Enhanced CO line ratios and broadening indicate shock heating.

Supports hadronic origin of gamma-rays with an estimated age of ~10,000 years.

Abstract

We have carried out a study of the interstellar medium (ISM) toward a shell-like supernova remnant SNR Puppis A by using the NANTEN CO and ATCA HI data. We synthesized a comprehensive picture of the SNR radiation by combining the ISM data with the gamma-ray and X-ray distributions. The ISM, both atomic and molecular gas, is dense and highly clumpy, and is distributed all around the SNR, but mainly in the north-east. The CO distribution revealed an enhanced line intensity ratio of CO($J$ = 2-1)/($J$ = 1-0) transitions as well as CO line broadening, which indicate shock heating/acceleration. The results support that Puppis A is located at 1.4 kpc, in the local arm. The ISM interacting with the SNR has a large mass of $\sim$10$^{4}$ $M_{\odot}$ which is dominated by HI, showing good spatial correspondence with the Fermi-LAT gamma-ray image. This favors the hadronic origin of the gamma-rays, while additional contribution of the leptonic component is not excluded. The distribution of the X-ray ionization timescales within the shell suggests that the shock front ionized various parts of the ISM at epochs ranging over a few to ten 1000 yr. We therefore suggest that the age of the SNR is around 10$^{4}$ yr as given by the largest ionization timescale. We estimate the total cosmic ray energy $W_{\rm p}$ to be 10$^{47}$ erg, which is well placed in the cosmic-ray escaping phase of an age-$W_{\rm p}$ plot including more than ten SNRs.