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EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8–6.3

  • Authors: Miroslav D. Filipović, Shi Dai, Bojan Arbutina, Natasha Hurley-Walker, Robert Brose, Werner Becker, Hidetoshi Sano, Dejan Urošević, T. H. Jarrett, Andrew M. Hopkins, Rami Z. E. Alsaberi, R. Alsulami, Cristobal Bordiu, Brianna Ball, Filomena Bufano, Christopher Burger-Scheidlin, Evan Crawford, Jayanne English, Frank Haberl, Adriano Ingallinera, Anna D. Kapinska, Patrick J. Kavanagh, Bärbel S. Koribalski, Roland Kothes, Sanja Lazarević, Jonathan Mackey, Gavin Rowell, Denis Leahy, Sara Loru, Peter J. Macgregor, Luciano Nicastro, Ray P. Norris, Simone Riggi, Manami Sasaki, Milorad Stupar, Corrado Trigilio, Grazia Umana, Tessa Vernstrom, Branislav Vukotić

Miroslav D. Filipović et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 6.

(a) Intensity distribution of H I obtained from HI4PI (HI4PI Collaboration et al. 2016). The integration velocity range is from −2.5 to 9.1 km s−1. The superposed contours indicate the intensity of the radio continuum. (b–c) Position–velocity diagrams of H I. The H I intensity is integrated from 157.°70 to 159.°15 in R.A. for panel (b) and from −65.°08 to −64.°54 in decl. for panel (c). The white dashed curve and yellow solid box in the position–velocity diagrams indicate candidates of a H I expanding shell and a high-velocity wing (see the text).

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