Fig. 13.
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Neutral hydrogen cavity west of the UJT-1 stellar wake. Map of the brightness temperature as detected in the EBHIS (Winkel et al. 2016) in the channel corresponding to an LSR velocity of −14 km s−1. A deep minimum lies west near the UJT-1 stellar wake. The blue-green map corresponds to the radio emission at 20 cm from CGPS, which might be attributed to an unpublished old supernova remnant that is likely to interact with dust particles in the wake.
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