A Detailed Study of the Interstellar Protons toward the TeV gamma-Ray SNR RX J0852.0-4622 (G266.2-1.2, Vela Jr.): The Third Case of the gamma-Ray and ISM Spatial Correspondence
We present a new analysis of the interstellar protons toward the TeV γ-ray SNR RX J0852.0−4622 (G266.2−1.2, Vela Jr.). We used the NANTEN2 12CO(J = 1–0) and Australia Telescope Compact Array and Parkes H i data sets in order to derive the molecular and atomic gas associated with the TeV γ-ray shell of the SNR. We find that atomic gas over a velocity range from V LSR = −4 to 50 km s−1 or 60 km s−1 is associated with the entire SNR, while molecular gas is associated with a limited portion of the...[Show more]
|Collections||ANU Research Publications|
|Source:||The Astrophysical Journal|
|Access Rights:||Open Access|
|01_Fukui_A_Detailed_Study_of_the_2017.pdf||8.65 MB||Adobe PDF|
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