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• W2897625566 abstract "The shell-type TeV source HESS J1912+101 was tentatively identified as an old supernova remnant, but is missing counterparts at radio and other frequencies. We analysed the Sino-German Urumqi $lambda$6 cm survey and the Effelsberg $lambda$11 cm and $lambda$21 cm surveys to identify radio emission from HESS J1912+101 to clarify the question of a supernova origin. We find a partial shell of excessive polarisation at $lambda$6 cm at the periphery of HESS J1912+101. At $lambda$11 cm, its polarised emission is faint and suffers from depolarisation, while at $lambda$21 cm, no related polarisation is seen. We could not separate the shell's total intensity signal from the confusing intense diffuse emission from the inner Galactic plane. However, a high-percentage polarisation of the shell's synchrotron emission is indicated. Our results support earlier suggestions that HESS J1912+101 is an old supernova remnant. The synchrotron emission is highly polarised, which is typical for evolved supernova remnants of low surface-brightness." @default.
• W2897625566 created "2018-10-26" @default.
• W2897625566 creator A5016412928 @default.
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• W2897625566 date "2019-03-01" @default.
• W2897625566 modified "2023-10-14" @default.
• W2897625566 title "Polarised radio emission associated with HESS J1912+101" @default.
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• W2897625566 doi "https://doi.org/10.1088/1674-4527/19/3/45" @default.
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