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G181.1+9.5, a new high-latitude low-surface brightness supernova remnant

By Roland Kothes, Patricia Reich, Tyler J. Foster and Wolfgang Reich

Abstract

Context. More than 90% of the known Milky Way supernova remnants (SNRs) are within 5° of the Galactic plane. The discovery of the new high-latitude SNR G181.1+9.5 will give us the opportunity to learn more about the environment and magnetic field at the interface between disk and halo of our Galaxy. Aims. We present the discovery of SNR G181.1+9.5, a new high-latitude SNR, serendipitously discovered in an ongoing survey of the Galactic anti-centre High-Velocity Cloud complex, observed with the DRAO Synthesis Telescope in the 21 cm radio continuum and H 

Topics: polarization, ISM: magnetic fields, ISM: supernova remnants, ISM: individual objects: G181.1+9.5
Publisher: EDP Sciences
DOI identifier: 10.1051/0004-6361/201629848
OAI identifier: oai:edpsciences.org:dkey/10.1051/0004-6361/201629848
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