Discovery of a molecular cloud possibly associated with the youngest Galactic SNR G1.9+0.3
Rei Enokiya, Hidetoshi Sano, Miroslav D. Filipovic, Rami Z. E., Alsaberi, Tsuyoshi Inoue And Tomoharu Oka

TL;DR
This study identifies a molecular cloud likely associated with the youngest Galactic supernova remnant G1.9+0.3, revealing how shock interaction with dense interstellar matter causes anisotropic expansion and provides insights into the remnant's environment.
Contribution
First direct evidence linking a molecular cloud to G1.9+0.3, demonstrating shock deceleration due to dense interstellar medium interaction.
Findings
The -1 km s-1 cloud is likely associated with G1.9+0.3.
The cloud shows a cavity structure coinciding with the SNR.
Interaction with the cloud causes anisotropic expansion of the SNR.
Abstract
The youngest known Galactic supernova remnant (SNR) G1.9+0.3 has high-velocity supernova shock beyond 10000 km s-1, and it is considered to be one of the major candidates of a PeVatron. Despite these outstanding properties, the surrounding interstellar matter of this object is poorly understood. We investigated the interstellar gas toward G1.9+0.3 using the 12CO(J=3-2) data with the angular resolution of 15" obtained by the CHIMPS2 survey by the James Clerk Maxwell Telescope, and discovered three individual clouds at -1, 7, and 45 km s-1. From its morphological and velocity structures, the -1 km s-1 cloud, having the largest velocity width >20 km s-1 and located at the distance of the Galactic Center, is possibly associated with the SNR. The associated cloud shows a cavity structure both in space and velocity and coincides well with the SNR. We found that the associated cloud has higher…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Ionosphere and magnetosphere dynamics
