Molecular and Atomic Gas toward HESS J1745-303 in the Galactic Center: Further Support for the Hadronic Scenario
Takahiro Hayakawa, Kazufumi Torii, Rei Enokiya, Takanobu Amano and, Yasuo Fukui

TL;DR
This study supports a hadronic origin for gamma-ray emissions from HESS J1745-303 by analyzing molecular and atomic gas data, estimating cosmic-ray proton energies, and exploring potential acceleration mechanisms near the Galactic Center.
Contribution
It provides new evidence linking interstellar gas distributions with gamma-ray sources and proposes a novel acceleration mechanism involving turbulence in the Galactic Center region.
Findings
Molecular gas MG358.9-0.5 aligns with the northern gamma-ray peak.
Atomic HI gas may be associated with the southern gamma-ray emission.
Estimated cosmic-ray proton energy is 6x10^{48} ergs.
Abstract
We have compared the TeV gamma-rays with the new 12CO J=2-1 data toward HESS J1745-303 in the Galactic center and confirmed that the molecular gas MG358.9-0.5 toward (l, b)=(358.9, -0.5 at VLSR=-100-0 km s-1 shows a reasonable positional agreement with the primary peak (northern part) of the gamma-ray source. For the southern part of HESS J1745-303, we see no CO counterpart, whereas the HI gas in the Parkes 21 cm HI dataset shows a possible counterpart to the gamma-ray source. This HI gas may be optically thick as supported by the HI line shape similar to the optically thick 12CO. We estimate the total mass of interstellar protons including both the molecular and atomic gas to be 2x10^6 Mo and the cosmic-ray proton energy to be 6x10^{48} ergs in the hadronic scenario. We discuss possible origins of the cosmic-ray protons including the nearby SNR G359.1-0.5. The SNR may be able to…
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