HIGHLIGHTS
- who: Veronese Simone et al. from the Netherlands Institute for Radio (ASTRON), Oude Hoogeveensedijk, PD Dwingeloo, The Netherlands Kapteyn Astronomical Institute, University of Groningen, , AV Groningen, The Netherlands have published the paper: Extended neutral hydrogen filamentary network in NGC, in the Journal: (JOURNAL)
- what: In the bottom right the authors show the 5200 u00d7 4900 beam. The non-co-rotating gas can be easily identified, as the authors show in Fig 3. The result is given in Fig 4, where the authors show the overlay between the galaxy emission and the GBT detection (left panel . . .
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